N3372V01MP0810
Mystic Mountain - Matte Paper - 8x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MP1010
Mystic Mountain - Matte Paper - 10x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MP1212
Mystic Mountain - Matte Paper - 12x12
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MP1216
Mystic Mountain - Matte Paper - 12x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MP1218
Mystic Mountain - Matte Paper - 12x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
20.00
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N3372V01MP1414
Mystic Mountain - Matte Paper - 14x14
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
20.00
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N3372V01MP1616
Mystic Mountain - Matte Paper - 16x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
22.00
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N3372V01MP1620
Mystic Mountain - Matte Paper - 16x20
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
24.00
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N3372V01MP1818
Mystic Mountain - Matte Paper - 18x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
24.00
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N3372V01MP1824
Mystic Mountain - Matte Paper - 18x24
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MP2436
Mystic Mountain - Matte Paper - 24x36
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
36.00
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N3372V01MF0810
Mystic Mountain - Matte Framed - 8x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
36.00
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N3372V01MF1010
Mystic Mountain - Matte Framed - 10x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
42.00
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N3372V01MF1212
Mystic Mountain - Matte Framed - 12x12
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
48.00
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N3372V01MF1216
Mystic Mountain - Matte Framed - 12x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
54.00
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N3372V01MF1218
Mystic Mountain - Matte Framed - 12x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
60.00
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N3372V01MF1414
Mystic Mountain - Matte Framed - 14x14
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MF1616
Mystic Mountain - Matte Framed - 16x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
66.00
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N3372V01MF1620
Mystic Mountain - Matte Framed - 16x20
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MF1818
Mystic Mountain - Matte Framed - 18x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01MF1824
Mystic Mountain - Matte Framed - 18x24
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
84.00
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N3372V01MF2436
Mystic Mountain - Matte Framed - 24x36
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
120.00
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N3372V01PP0810
Mystic Mountain - Photo Paper - 8x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PP1010
Mystic Mountain - Photo Paper - 10x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PP1212
Mystic Mountain - Photo Paper - 12x12
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PP1216
Mystic Mountain - Photo Paper - 12x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PP1218
Mystic Mountain - Photo Paper - 12x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
24.00
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N3372V01PP1414
Mystic Mountain - Photo Paper - 14x14
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
24.00
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N3372V01PP1616
Mystic Mountain - Photo Paper - 16x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
26.00
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N3372V01PP1620
Mystic Mountain - Photo Paper - 16x20
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
28.00
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N3372V01PP1818
Mystic Mountain - Photo Paper - 18x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
28.00
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N3372V01PP1824
Mystic Mountain - Photo Paper - 18x24
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PP2436
Mystic Mountain - Photo Paper - 24x36
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
40.00
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N3372V01PF0810
Mystic Mountain - Photo Framed - 8x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
46.00
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N3372V01PF1010
Mystic Mountain - Photo Framed - 10x10
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
52.00
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N3372V01PF1212
Mystic Mountain - Photo Framed - 12x12
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
58.00
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N3372V01PF1216
Mystic Mountain - Photo Framed - 12x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
64.00
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N3372V01PF1218
Mystic Mountain - Photo Framed - 12x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
70.00
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N3372V01PF1414
Mystic Mountain - Photo Framed - 14x14
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PF1616
Mystic Mountain - Photo Framed - 16x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
76.00
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N3372V01PF1620
Mystic Mountain - Photo Framed - 16x20
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PF1818
Mystic Mountain - Photo Framed - 18x18
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PF1824
Mystic Mountain - Photo Framed - 18x24
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01PF2436
Mystic Mountain - Photo Framed - 24x36
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
126.00
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N3372V01CA1212
Mystic Mountain - Canvas - 12x12
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01CA1216
Mystic Mountain - Canvas - 12x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
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N3372V01CA1616
Mystic Mountain - Canvas - 16x16
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
58.00
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N3372V01CA1620
Mystic Mountain - Canvas - 16x20
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
60.00
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N3372V01CA1824
Mystic Mountain - Canvas - 18x24
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
70.00
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N3372V01CA2436
Mystic Mountain - Canvas - 24x36
A Mystic Mountain of dust and gas rises within the Carina Nebula The top of a three-light-year tall pillar of cool hydrogen laced with dust rises from the wall of the nebula and is being worn away by the radiation of nearby stars. From the peaks, stars within the pillar unleash jets of streaming gas. This photo, marking Hubble's 20th anniversary, is of a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. The pillar is also being pushed apart by infant stars from within, as they fire off jets of gas that can be seen streaming from the peaks like arrows flying through the air. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: HH 901 and HH 902 in the Carina Nebula Release Date: Apr 15, 2010 Image Credits: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)
100.00
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N2070V00MP0810
30 Doradus - Matte Paper - 8x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
12.00
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N2070V00MP1010
30 Doradus - Matte Paper - 10x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
14.00
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N2070V00MP1212
30 Doradus - Matte Paper - 12x12
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
16.00
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N2070V00MP1216
30 Doradus - Matte Paper - 12x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
18.00
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N2070V00MP1218
30 Doradus - Matte Paper - 12x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
20.00
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N2070V00MP1414
30 Doradus - Matte Paper - 14x14
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
20.00
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N2070V00MP1616
30 Doradus - Matte Paper - 16x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
22.00
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N2070V00MP1620
30 Doradus - Matte Paper - 16x20
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
24.00
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N2070V00MP1818
30 Doradus - Matte Paper - 18x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
24.00
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N2070V00MP1824
30 Doradus - Matte Paper - 18x24
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
28.00
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N2070V00MP2436
30 Doradus - Matte Paper - 24x36
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
36.00
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N2070V00MF0810
30 Doradus - Matte Framed - 8x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
36.00
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N2070V00MF1010
30 Doradus - Matte Framed - 10x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
42.00
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N2070V00MF1212
30 Doradus - Matte Framed - 12x12
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
48.00
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N2070V00MF1216
30 Doradus - Matte Framed - 12x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
54.00
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N2070V00MF1218
30 Doradus - Matte Framed - 12x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
60.00
https://posternauts.com/products/30-doradus?variant=35410686472
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N2070V00MF1414
30 Doradus - Matte Framed - 14x14
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
60.00
https://posternauts.com/products/30-doradus?variant=35410686536
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https://posternauts.com/cdn/shop/products/30Dor-frame-18x18_medium.png?v=1496945021,
N2070V00MF1616
30 Doradus - Matte Framed - 16x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
66.00
https://posternauts.com/products/30-doradus?variant=35410686600
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N2070V00MF1620
30 Doradus - Matte Framed - 16x20
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
72.00
https://posternauts.com/products/30-doradus?variant=35410686664
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N2070V00MF1818
30 Doradus - Matte Framed - 18x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
72.00
https://posternauts.com/products/30-doradus?variant=35410686728
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N2070V00MF1824
30 Doradus - Matte Framed - 18x24
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
84.00
https://posternauts.com/products/30-doradus?variant=35410686792
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N2070V00MF2436
30 Doradus - Matte Framed - 24x36
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
120.00
https://posternauts.com/products/30-doradus?variant=35410686856
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N2070V00PP0810
30 Doradus - Photo Paper - 8x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
16.00
https://posternauts.com/products/30-doradus?variant=35410686920
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N2070V00PP1010
30 Doradus - Photo Paper - 10x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
18.00
https://posternauts.com/products/30-doradus?variant=35410686984
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N2070V00PP1212
30 Doradus - Photo Paper - 12x12
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
20.00
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N2070V00PP1216
30 Doradus - Photo Paper - 12x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
22.00
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N2070V00PP1218
30 Doradus - Photo Paper - 12x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
24.00
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N2070V00PP1414
30 Doradus - Photo Paper - 14x14
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
24.00
https://posternauts.com/products/30-doradus?variant=35410687240
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N2070V00PP1616
30 Doradus - Photo Paper - 16x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
26.00
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N2070V00PP1620
30 Doradus - Photo Paper - 16x20
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
28.00
https://posternauts.com/products/30-doradus?variant=35410687368
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N2070V00PP1818
30 Doradus - Photo Paper - 18x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
28.00
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N2070V00PP1824
30 Doradus - Photo Paper - 18x24
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
34.00
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N2070V00PP2436
30 Doradus - Photo Paper - 24x36
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
40.00
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N2070V00PF0810
30 Doradus - Photo Framed - 8x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
46.00
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N2070V00PF1010
30 Doradus - Photo Framed - 10x10
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
52.00
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https://posternauts.com/cdn/shop/products/30Dor-frame-18x18_medium.png?v=1496945021,
N2070V00PF1212
30 Doradus - Photo Framed - 12x12
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
58.00
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N2070V00PF1216
30 Doradus - Photo Framed - 12x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
64.00
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N2070V00PF1218
30 Doradus - Photo Framed - 12x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
70.00
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N2070V00PF1414
30 Doradus - Photo Framed - 14x14
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
70.00
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N2070V00PF1616
30 Doradus - Photo Framed - 16x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
76.00
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N2070V00PF1620
30 Doradus - Photo Framed - 16x20
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
82.00
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N2070V00PF1818
30 Doradus - Photo Framed - 18x18
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
82.00
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N2070V00PF1824
30 Doradus - Photo Framed - 18x24
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
100.00
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N2070V00PF2436
30 Doradus - Photo Framed - 24x36
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
126.00
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N2070V00CA1212
30 Doradus - Canvas - 12x12
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
54.00
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N2070V00CA1216
30 Doradus - Canvas - 12x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
56.00
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N2070V00CA1616
30 Doradus - Canvas - 16x16
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
58.00
https://posternauts.com/products/30-doradus?variant=35410688712
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N2070V00CA1620
30 Doradus - Canvas - 16x20
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
60.00
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N2070V00CA1824
30 Doradus - Canvas - 18x24
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
70.00
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N2070V00CA2436
30 Doradus - Canvas - 24x36
This image from the 22nd anniversary of Hubble shows a turbulent star-making region. In the heart of the Tarantula nebula lies 30 Doradus, the brightest star-forming region in our galactic neighborhood. It is home to several million young stars; including the most massive stars ever seen. The nebula is situated 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070 Release Date: Apr 14, 2012 Image Credits: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
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N0346V00MP0810
Infant Stars in the Small Magellanic Cloud - Matte Paper - 8x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00MP1010
Infant Stars in the Small Magellanic Cloud - Matte Paper - 10x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00MP1212
Infant Stars in the Small Magellanic Cloud - Matte Paper - 12x12
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00MP1216
Infant Stars in the Small Magellanic Cloud - Matte Paper - 12x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00MP1218
Infant Stars in the Small Magellanic Cloud - Matte Paper - 12x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
20.00
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N0346V00MP1414
Infant Stars in the Small Magellanic Cloud - Matte Paper - 14x14
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
20.00
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N0346V00MP1616
Infant Stars in the Small Magellanic Cloud - Matte Paper - 16x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00MP1620
Infant Stars in the Small Magellanic Cloud - Matte Paper - 16x20
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
24.00
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N0346V00MP1818
Infant Stars in the Small Magellanic Cloud - Matte Paper - 18x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
24.00
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N0346V00MP1824
Infant Stars in the Small Magellanic Cloud - Matte Paper - 18x24
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00MP2436
Infant Stars in the Small Magellanic Cloud - Matte Paper - 24x36
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
36.00
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N0346V00MF0810
Infant Stars in the Small Magellanic Cloud - Matte Framed - 8x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
36.00
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N0346V00MF1010
Infant Stars in the Small Magellanic Cloud - Matte Framed - 10x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
42.00
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N0346V00MF1212
Infant Stars in the Small Magellanic Cloud - Matte Framed - 12x12
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
48.00
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N0346V00MF1216
Infant Stars in the Small Magellanic Cloud - Matte Framed - 12x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
54.00
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N0346V00MF1218
Infant Stars in the Small Magellanic Cloud - Matte Framed - 12x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
60.00
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N0346V00MF1414
Infant Stars in the Small Magellanic Cloud - Matte Framed - 14x14
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
60.00
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N0346V00MF1616
Infant Stars in the Small Magellanic Cloud - Matte Framed - 16x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
66.00
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N0346V00MF1620
Infant Stars in the Small Magellanic Cloud - Matte Framed - 16x20
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
72.00
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N0346V00MF1818
Infant Stars in the Small Magellanic Cloud - Matte Framed - 18x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
72.00
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N0346V00MF1824
Infant Stars in the Small Magellanic Cloud - Matte Framed - 18x24
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
84.00
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N0346V00MF2436
Infant Stars in the Small Magellanic Cloud - Matte Framed - 24x36
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
120.00
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N0346V00PP0810
Infant Stars in the Small Magellanic Cloud - Photo Paper - 8x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
16.00
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N0346V00PP1010
Infant Stars in the Small Magellanic Cloud - Photo Paper - 10x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP1212
Infant Stars in the Small Magellanic Cloud - Photo Paper - 12x12
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP1216
Infant Stars in the Small Magellanic Cloud - Photo Paper - 12x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP1218
Infant Stars in the Small Magellanic Cloud - Photo Paper - 12x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP1414
Infant Stars in the Small Magellanic Cloud - Photo Paper - 14x14
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP1616
Infant Stars in the Small Magellanic Cloud - Photo Paper - 16x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP1620
Infant Stars in the Small Magellanic Cloud - Photo Paper - 16x20
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP1818
Infant Stars in the Small Magellanic Cloud - Photo Paper - 18x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
28.00
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N0346V00PP1824
Infant Stars in the Small Magellanic Cloud - Photo Paper - 18x24
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PP2436
Infant Stars in the Small Magellanic Cloud - Photo Paper - 24x36
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PF0810
Infant Stars in the Small Magellanic Cloud - Photo Framed - 8x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PF1010
Infant Stars in the Small Magellanic Cloud - Photo Framed - 10x10
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
52.00
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N0346V00PF1212
Infant Stars in the Small Magellanic Cloud - Photo Framed - 12x12
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PF1216
Infant Stars in the Small Magellanic Cloud - Photo Framed - 12x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N0346V00PF1218
Infant Stars in the Small Magellanic Cloud - Photo Framed - 12x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
70.00
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N0346V00PF1414
Infant Stars in the Small Magellanic Cloud - Photo Framed - 14x14
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
70.00
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N0346V00PF1616
Infant Stars in the Small Magellanic Cloud - Photo Framed - 16x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
76.00
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N0346V00PF1620
Infant Stars in the Small Magellanic Cloud - Photo Framed - 16x20
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
82.00
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N0346V00PF1818
Infant Stars in the Small Magellanic Cloud - Photo Framed - 18x18
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
82.00
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N0346V00PF1824
Infant Stars in the Small Magellanic Cloud - Photo Framed - 18x24
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
100.00
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N0346V00PF2436
Infant Stars in the Small Magellanic Cloud - Photo Framed - 24x36
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
126.00
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N0346V00CA1212
Infant Stars in the Small Magellanic Cloud - Canvas - 12x12
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
54.00
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N0346V00CA1216
Infant Stars in the Small Magellanic Cloud - Canvas - 12x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
56.00
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N0346V00CA1616
Infant Stars in the Small Magellanic Cloud - Canvas - 16x16
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
58.00
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N0346V00CA1620
Infant Stars in the Small Magellanic Cloud - Canvas - 16x20
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
60.00
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N0346V00CA1824
Infant Stars in the Small Magellanic Cloud - Canvas - 18x24
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
70.00
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N0346V00CA2436
Infant Stars in the Small Magellanic Cloud - Canvas - 24x36
This group of baby stars still forming from collapsing gas clouds have not yet ignited their hydrogen fuel. The Small Magellanic Cloud is a satellite galaxy of the Milky Way and Hubble has uncovered a population of embryonic stars within. Hubble provides a crisp view of these young stars as they coalesce out of gravitationally collapsing gas clouds. The stars have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 346 Release Date: Jan 12, 2005 Image Credits: NASA, ESA, and A. Nota (STScI/ESA)
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N6302V00MP0810
Butterfly Nebula - Matte Paper - 8x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1010
Butterfly Nebula - Matte Paper - 10x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1212
Butterfly Nebula - Matte Paper - 12x12
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1216
Butterfly Nebula - Matte Paper - 12x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1218
Butterfly Nebula - Matte Paper - 12x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1414
Butterfly Nebula - Matte Paper - 14x14
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1616
Butterfly Nebula - Matte Paper - 16x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1620
Butterfly Nebula - Matte Paper - 16x20
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1818
Butterfly Nebula - Matte Paper - 18x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP1824
Butterfly Nebula - Matte Paper - 18x24
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MP2436
Butterfly Nebula - Matte Paper - 24x36
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF0810
Butterfly Nebula - Matte Framed - 8x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1010
Butterfly Nebula - Matte Framed - 10x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1212
Butterfly Nebula - Matte Framed - 12x12
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1216
Butterfly Nebula - Matte Framed - 12x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1218
Butterfly Nebula - Matte Framed - 12x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1414
Butterfly Nebula - Matte Framed - 14x14
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1616
Butterfly Nebula - Matte Framed - 16x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1620
Butterfly Nebula - Matte Framed - 16x20
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1818
Butterfly Nebula - Matte Framed - 18x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF1824
Butterfly Nebula - Matte Framed - 18x24
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00MF2436
Butterfly Nebula - Matte Framed - 24x36
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP0810
Butterfly Nebula - Photo Paper - 8x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1010
Butterfly Nebula - Photo Paper - 10x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1212
Butterfly Nebula - Photo Paper - 12x12
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1216
Butterfly Nebula - Photo Paper - 12x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1218
Butterfly Nebula - Photo Paper - 12x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1414
Butterfly Nebula - Photo Paper - 14x14
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1616
Butterfly Nebula - Photo Paper - 16x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1620
Butterfly Nebula - Photo Paper - 16x20
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1818
Butterfly Nebula - Photo Paper - 18x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP1824
Butterfly Nebula - Photo Paper - 18x24
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PP2436
Butterfly Nebula - Photo Paper - 24x36
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF0810
Butterfly Nebula - Photo Framed - 8x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1010
Butterfly Nebula - Photo Framed - 10x10
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1212
Butterfly Nebula - Photo Framed - 12x12
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1216
Butterfly Nebula - Photo Framed - 12x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1218
Butterfly Nebula - Photo Framed - 12x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1414
Butterfly Nebula - Photo Framed - 14x14
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1616
Butterfly Nebula - Photo Framed - 16x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1620
Butterfly Nebula - Photo Framed - 16x20
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1818
Butterfly Nebula - Photo Framed - 18x18
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF1824
Butterfly Nebula - Photo Framed - 18x24
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00PF2436
Butterfly Nebula - Photo Framed - 24x36
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
126.00
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N6302V00CA1212
Butterfly Nebula - Canvas - 12x12
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00CA1216
Butterfly Nebula - Canvas - 12x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00CA1616
Butterfly Nebula - Canvas - 16x16
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00CA1620
Butterfly Nebula - Canvas - 16x20
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00CA1824
Butterfly Nebula - Canvas - 18x24
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N6302V00CA2436
Butterfly Nebula - Canvas - 24x36
Gas released by a dying star races across space at more than 600,000 miles an hour. This Butterfly Nebula is also known as NGC 6302 or the Bug Nebula which rests in the constellation Scorpius. The burst of energy released from a dying star pulls and energizes gas along with it, forming a delicate shape like a butterfly or an hourglass. Its central star, a recently discovered white dwarf, is one of the hottest stars in the galaxy, with a surface temperature over 200,000 K. Amazingly, this object has been know since at least 1888 and the earliest known study of it took place in 1907, long before Hubble brought us this spectacular view. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 6302 (Butterfly Nebula, Bug Nebula) Release Date: Sep 18, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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RVA01V00MP1218
Viking 40 Year Anniversary - Matte Paper - 12x18
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00MP2436
Viking 40 Year Anniversary - Matte Paper - 24x36
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00MF1218
Viking 40 Year Anniversary - Matte Framed - 12x18
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00MF2436
Viking 40 Year Anniversary - Matte Framed - 24x36
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00PP1218
Viking 40 Year Anniversary - Photo Paper - 12x18
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00PP2436
Viking 40 Year Anniversary - Photo Paper - 24x36
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00PF1218
Viking 40 Year Anniversary - Photo Framed - 12x18
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00PF2436
Viking 40 Year Anniversary - Photo Framed - 24x36
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVA01V00CA2436
Viking 40 Year Anniversary - Canvas - 24x36
Both the Viking 1 and Viking 2 Orbiters collected years of high-resolution imagery and scientific data about Mars and its moons. On July 20, 1976, NASA's Viking 1 Lander touched down to take its first picture of the dusty, rocky surface of Mars. It relayed the historic image back to Earth and began years of data collection. The Viking 2 Lander followed on September 3, 1976. Both blazed the trail to Mars and we have returned many times to the Red Planet since. Enjoy this retro-style artwork which commemorates the 40th anniversary of NASA's Viking 1 and 2 missions to Mars! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA
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RVF14V00MP1218
PSO J318.5-22 - NASA Visions of the Future - Matte Paper - 12x18
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00MP2436
PSO J318.5-22 - NASA Visions of the Future - Matte Paper - 24x36
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00MF1218
PSO J318.5-22 - NASA Visions of the Future - Matte Framed - 12x18
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00MF2436
PSO J318.5-22 - NASA Visions of the Future - Matte Framed - 24x36
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00PP1218
PSO J318.5-22 - NASA Visions of the Future - Photo Paper - 12x18
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00PP2436
PSO J318.5-22 - NASA Visions of the Future - Photo Paper - 24x36
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00PF1218
PSO J318.5-22 - NASA Visions of the Future - Photo Framed - 12x18
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00PF2436
PSO J318.5-22 - NASA Visions of the Future - Photo Framed - 24x36
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF14V00CA2436
PSO J318.5-22 - NASA Visions of the Future - Canvas - 24x36
Wandering alone in the galaxy, rogue planets do not orbit a parent star. PSO J318.5-22 was discovered in October 2013 using direct imaging and belongs to a special class of planets called rogue, or free-floating, planets. Not much is known about how these planets come to exist, but they may be either failed stars or planets ejected from very young systems after an encounter with another planet. These rogue planets glow faintly from the heat of their formation, but once they cool down they will be completely in the dark. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF10V00MP1218
51 Pegasus b - NASA Visions of the Future - Matte Paper - 12x18
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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RVF10V00MP2436
51 Pegasus b - NASA Visions of the Future - Matte Paper - 24x36
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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51 Pegasus b - NASA Visions of the Future - Matte Framed - 12x18
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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51 Pegasus b - NASA Visions of the Future - Matte Framed - 24x36
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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51 Pegasus b - NASA Visions of the Future - Photo Paper - 12x18
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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51 Pegasus b - NASA Visions of the Future - Photo Paper - 24x36
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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51 Pegasus b - NASA Visions of the Future - Photo Framed - 12x18
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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51 Pegasus b - NASA Visions of the Future - Photo Framed - 24x36
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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51 Pegasus b - NASA Visions of the Future - Canvas - 24x36
In 1995, scientists discovered 51 Pegasi b and changed the way we see the universe and our place in it forever. There is debate over which exoplanet was discovered is considered the "first," one stands out from the rest. The exoplanet is about half the mass of Jupiter, with a seemingly impossible, star-hugging orbit of only 4.2 Earth days. Not only was it the first planet confirmed to orbit a sun-like star, it also ushered in a whole new class of planets called Hot Jupiters: hot, massive planets orbiting closer to their stars than Mercury. Today, powerful observatories like NASA's Kepler space telescope will continue the hunt of distant planets. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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Work the Night Shift - NASA Mars Explorers Wanted - Matte Paper - 12x18
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Matte Paper - 24x36
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Matte Framed - 12x18
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Matte Framed - 24x36
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Photo Paper - 12x18
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Photo Paper - 24x36
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Photo Framed - 12x18
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Photo Framed - 24x36
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Work the Night Shift - NASA Mars Explorers Wanted - Canvas - 24x36
Interested in working the night shift on the Martian moon Phobos? If you lived on the moon Phobos, you would have an office with an amazing view, mining for resources with Mars floating in the night sky. Settlers below on Mars would look up to see Phobos rise and set not just once, but twice in one day! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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N5194V00MP0810
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 8x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 10x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 12x12
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 12x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 12x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 14x14
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MP1616
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 16x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MP1620
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 16x20
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MP1818
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 18x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MP1824
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 18x24
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MP2436
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Paper - 24x36
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF0810
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 8x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1010
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 10x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1212
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 12x12
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1216
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 12x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1218
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 12x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1414
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 14x14
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1616
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 16x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1620
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 16x20
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1818
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 18x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF1824
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 18x24
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00MF2436
Whirlpool Galaxy and Companion Galaxy - M51 - Matte Framed - 24x36
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP0810
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 8x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1010
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 10x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1212
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 12x12
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1216
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 12x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1218
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 12x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1414
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 14x14
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1616
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 16x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1620
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 16x20
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1818
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 18x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP1824
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 18x24
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PP2436
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Paper - 24x36
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF0810
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 8x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1010
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 10x10
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1212
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 12x12
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1216
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 12x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1218
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 12x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1414
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 14x14
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1616
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 16x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1620
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 16x20
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1818
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 18x18
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF1824
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 18x24
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00PF2436
Whirlpool Galaxy and Companion Galaxy - M51 - Photo Framed - 24x36
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00CA1212
Whirlpool Galaxy and Companion Galaxy - M51 - Canvas - 12x12
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00CA1216
Whirlpool Galaxy and Companion Galaxy - M51 - Canvas - 12x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
56.00
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N5194V00CA1616
Whirlpool Galaxy and Companion Galaxy - M51 - Canvas - 16x16
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00CA1620
Whirlpool Galaxy and Companion Galaxy - M51 - Canvas - 16x20
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00CA1824
Whirlpool Galaxy and Companion Galaxy - M51 - Canvas - 18x24
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
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N5194V00CA2436
Whirlpool Galaxy and Companion Galaxy - M51 - Canvas - 24x36
The Whirlpool spiral galaxy M51, is one of the most well-known objects ever observed by Hubble. On its 15th anniversary, Hubble released this new view of M51, which was among the largest and sharpest images Hubble had ever taken with its newest camera, the Advanced Camera for Surveys (ACS). This large Whirlpool Galaxy has sharply defined spiral arms which may be the result of the Whirlpool's gravitational tug-of-war with the smaller companion galaxy nearby. The image showcases classic features of spiral galaxies, from the curving arms where newborn stars spin, to the yellowish central core which serves as the home for older stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Whirlpool Galaxy, M51, NGC 5194/5 Release date: Apr 25, 2005 Image Credits: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
100.00
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N3247V00MP0810
Westerlund 2 - Matte Paper - 8x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1010
Westerlund 2 - Matte Paper - 10x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1212
Westerlund 2 - Matte Paper - 12x12
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1216
Westerlund 2 - Matte Paper - 12x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1218
Westerlund 2 - Matte Paper - 12x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1414
Westerlund 2 - Matte Paper - 14x14
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1616
Westerlund 2 - Matte Paper - 16x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
22.00
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N3247V00MP1620
Westerlund 2 - Matte Paper - 16x20
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1818
Westerlund 2 - Matte Paper - 18x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MP1824
Westerlund 2 - Matte Paper - 18x24
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
28.00
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N3247V00MP2436
Westerlund 2 - Matte Paper - 24x36
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
36.00
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N3247V00MF0810
Westerlund 2 - Matte Framed - 8x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
36.00
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N3247V00MF1010
Westerlund 2 - Matte Framed - 10x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
42.00
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N3247V00MF1212
Westerlund 2 - Matte Framed - 12x12
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
48.00
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N3247V00MF1216
Westerlund 2 - Matte Framed - 12x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MF1218
Westerlund 2 - Matte Framed - 12x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MF1414
Westerlund 2 - Matte Framed - 14x14
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MF1616
Westerlund 2 - Matte Framed - 16x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MF1620
Westerlund 2 - Matte Framed - 16x20
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MF1818
Westerlund 2 - Matte Framed - 18x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MF1824
Westerlund 2 - Matte Framed - 18x24
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00MF2436
Westerlund 2 - Matte Framed - 24x36
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00PP0810
Westerlund 2 - Photo Paper - 8x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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N3247V00PP1010
Westerlund 2 - Photo Paper - 10x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
18.00
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N3247V00PP1212
Westerlund 2 - Photo Paper - 12x12
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
20.00
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https://posternauts.com/cdn/shop/products/ps58-poster-18x18_medium.png?v=1496951962,
N3247V00PP1216
Westerlund 2 - Photo Paper - 12x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
22.00
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https://posternauts.com/cdn/shop/products/ps58-poster-18x24_medium.png?v=1496951965,
N3247V00PP1218
Westerlund 2 - Photo Paper - 12x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
24.00
https://posternauts.com/products/westerlund-2?variant=35121426120
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https://posternauts.com/cdn/shop/products/ps58-poster-36x24_medium.png?v=1496443286,
N3247V00PP1414
Westerlund 2 - Photo Paper - 14x14
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
24.00
https://posternauts.com/products/westerlund-2?variant=35121426184
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https://posternauts.com/cdn/shop/products/ps58-poster-18x18_medium.png?v=1496951962,
N3247V00PP1616
Westerlund 2 - Photo Paper - 16x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
26.00
https://posternauts.com/products/westerlund-2?variant=35121426248
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https://posternauts.com/cdn/shop/products/ps58-poster-18x18_medium.png?v=1496951962,
N3247V00PP1620
Westerlund 2 - Photo Paper - 16x20
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
28.00
https://posternauts.com/products/westerlund-2?variant=35121426312
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https://posternauts.com/cdn/shop/products/ps58-poster-16x20_medium.png?v=1496951959,
N3247V00PP1818
Westerlund 2 - Photo Paper - 18x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
28.00
https://posternauts.com/products/westerlund-2?variant=35121426376
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https://posternauts.com/cdn/shop/products/ps58-poster-18x18_medium.png?v=1496951962,
N3247V00PP1824
Westerlund 2 - Photo Paper - 18x24
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
34.00
https://posternauts.com/products/westerlund-2?variant=35121426440
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https://posternauts.com/cdn/shop/products/ps58-poster-18x24_medium.png?v=1496951965,
N3247V00PP2436
Westerlund 2 - Photo Paper - 24x36
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
40.00
https://posternauts.com/products/westerlund-2?variant=35121426504
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https://posternauts.com/cdn/shop/products/ps58-poster-36x24_medium.png?v=1496443286,
N3247V00PF0810
Westerlund 2 - Photo Framed - 8x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
46.00
https://posternauts.com/products/westerlund-2?variant=35121426568
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https://posternauts.com/cdn/shop/products/ps58-frame-16x20_medium.png?v=1496951935,
N3247V00PF1010
Westerlund 2 - Photo Framed - 10x10
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
52.00
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https://posternauts.com/cdn/shop/products/ps58-frame-18x18_medium.png?v=1496951937,
N3247V00PF1212
Westerlund 2 - Photo Framed - 12x12
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
58.00
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https://posternauts.com/cdn/shop/products/ps58-frame-18x18_medium.png?v=1496951937,
N3247V00PF1216
Westerlund 2 - Photo Framed - 12x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
64.00
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https://posternauts.com/cdn/shop/products/ps58-frame-18x24_medium.png?v=1496951940,
N3247V00PF1218
Westerlund 2 - Photo Framed - 12x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
70.00
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https://posternauts.com/cdn/shop/products/ps58-frame-36x24_medium.png?v=1496443286,
N3247V00PF1414
Westerlund 2 - Photo Framed - 14x14
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
70.00
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https://posternauts.com/cdn/shop/products/ps58-frame-18x18_medium.png?v=1496951937,
N3247V00PF1616
Westerlund 2 - Photo Framed - 16x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
76.00
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https://posternauts.com/cdn/shop/products/ps58-frame-18x18_medium.png?v=1496951937,
N3247V00PF1620
Westerlund 2 - Photo Framed - 16x20
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
82.00
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https://posternauts.com/cdn/shop/products/ps58-frame-16x20_medium.png?v=1496951935,
N3247V00PF1818
Westerlund 2 - Photo Framed - 18x18
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
82.00
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https://posternauts.com/cdn/shop/products/ps58-frame-18x18_medium.png?v=1496951937,
N3247V00PF1824
Westerlund 2 - Photo Framed - 18x24
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
100.00
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https://posternauts.com/cdn/shop/products/ps58-frame-18x24_medium.png?v=1496951940,
N3247V00PF2436
Westerlund 2 - Photo Framed - 24x36
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
126.00
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https://posternauts.com/cdn/shop/products/ps58-frame-36x24_medium.png?v=1496443286,
N3247V00CA1212
Westerlund 2 - Canvas - 12x12
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
54.00
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https://posternauts.com/cdn/shop/products/ps58-canvas-16x16_medium.png?v=1496951915,
N3247V00CA1216
Westerlund 2 - Canvas - 12x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
56.00
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https://posternauts.com/cdn/shop/products/ps58-canvas-18x24_medium.png?v=1496951920,
N3247V00CA1616
Westerlund 2 - Canvas - 16x16
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
58.00
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N3247V00CA1620
Westerlund 2 - Canvas - 16x20
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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Westerlund 2 - Canvas - 18x24
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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Westerlund 2 - Canvas - 24x36
This relatively young, 2-million-year-old star cluster contains some of the hottest, brightest, and most massive stars in our galaxy. Westerlund 2 is a giant, sparkling cluster of about 3,000 stars in a raucous stellar breeding ground called Gum 29. It is located 20,000 light-years away from Earth in the constellation Carina. The largest stars unleash a torrent of ultraviolet light and hurricane-force winds that etch away the enveloping hydrogen gas cloud. This results in a celestial landscape of pillars, ridges, and valleys, unveiling some of nature's own fireworks. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Westerlund 2, Gum 29, NGC 3247 Release Date: Apr 23, 2015 Image Credits: NASA, ESA, A. Nota (ESA/STScI), and the Westerlund 2 Science Team
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We Need You - NASA Mars Explorers Wanted - Matte Paper - 12x18
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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We Need You - NASA Mars Explorers Wanted - Matte Paper - 24x36
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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We Need You - NASA Mars Explorers Wanted - Matte Framed - 12x18
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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REW08V00MF2436
We Need You - NASA Mars Explorers Wanted - Matte Framed - 24x36
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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REW08V00PP1218
We Need You - NASA Mars Explorers Wanted - Photo Paper - 12x18
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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We Need You - NASA Mars Explorers Wanted - Photo Paper - 24x36
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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REW08V00PF1218
We Need You - NASA Mars Explorers Wanted - Photo Framed - 12x18
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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We Need You - NASA Mars Explorers Wanted - Photo Framed - 24x36
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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We Need You - NASA Mars Explorers Wanted - Canvas - 24x36
We need you... for the Journey to Mars! It will take a lot of planing and preparation to get astronauts to Mars. Many resources will be needed for the Journey to Mars, but the most important thing is YOU! NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/KSC
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Venus - NASA Visions of the Future - Matte Paper - 12x18
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF04V00MP2436
Venus - NASA Visions of the Future - Matte Paper - 24x36
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF04V00MF1218
Venus - NASA Visions of the Future - Matte Framed - 12x18
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Venus - NASA Visions of the Future - Matte Framed - 24x36
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Venus - NASA Visions of the Future - Photo Paper - 12x18
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Venus - NASA Visions of the Future - Photo Paper - 24x36
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Venus - NASA Visions of the Future - Photo Framed - 12x18
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Venus - NASA Visions of the Future - Photo Framed - 24x36
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Venus - NASA Visions of the Future - Canvas - 24x36
When the surface of Venus is anything but pleasant, a floating city in the clouds may be only slightly less uncomfortable. Spacecraft now allow us the luxury to study planetary transits at times of our choosing from unique locations across the solar system. The rare science opportunity of observing these cosmic crossings has long inspired bold voyages to exotic vantage points, such as James Cook's trek to the South Pacific to watch Venus and Mercury cross the face of the Sun in 1769. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Valles Marineris - SpaceX Mars Travel - Matte Paper - 12x18
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Valles Marineris - SpaceX Mars Travel - Matte Paper - 24x36
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Valles Marineris - SpaceX Mars Travel - Matte Framed - 12x18
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Valles Marineris - SpaceX Mars Travel - Matte Framed - 24x36
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Valles Marineris - SpaceX Mars Travel - Photo Paper - 12x18
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Valles Marineris - SpaceX Mars Travel - Photo Framed - 12x18
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Valles Marineris - SpaceX Mars Travel - Photo Framed - 24x36
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Valles Marineris - SpaceX Mars Travel - Canvas - 24x36
Get your jet pack on and zip through the Martian landscape. Valles Marineris is the canyon system that runs along the equator of Mars. At seven-miles deep, it is four-times deeper than the Grand Canyon of Earth. Visitors might very well want to relax and fly through instead of hiking to the bottom. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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Trappist-1e - NASA Visions of the Future - Matte Paper - 12x18
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Matte Paper - 24x36
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Matte Framed - 12x18
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Matte Framed - 24x36
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Photo Paper - 12x18
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Photo Paper - 24x36
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Photo Framed - 12x18
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Photo Framed - 24x36
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Trappist-1e - NASA Visions of the Future - Canvas - 24x36
Trappist-1e is just one of seven planets together in close orbit around their star. Approximately 40 light-years from Earth, the planet Trappist-1e offers a heart-stopping view. The brilliant objects in its red sky, looming like larger and smaller versions of our own moon are not moons at all. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle close around their small, dim, red star. Any of them may harbor liquid water, but the fourth planet from the Trappist-1 star, is in the habitable zone. This system was revealed by the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) and NASA’s Spitzer Space Telescope and are also excellent targets for NASA’s James Webb Space Telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Matte Paper - 12x18
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Matte Paper - 24x36
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Matte Framed - 12x18
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Matte Framed - 24x36
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Photo Paper - 12x18
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Photo Paper - 24x36
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Photo Framed - 12x18
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Photo Framed - 24x36
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Titan - NASA Visions of the Future - Canvas - 24x36
Titan is a frigid and alien moon similar to our own planet billions of years ago. Saturn's largest moon, Titan, has a thick atmosphere with organic-rich chemistry. Its surface is shaped by rivers and lakes of liquid ethane and methane. Cold winds sculpt vast regions of hydrocarbon-rich dunes. There may even be cryovolcanoes of cold liquid water. NASA's Cassini orbiter was designed to see through the ever present haze of Titan to unravel the mysteries of this planet-like moon. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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NASA's Voyager mission took advantage of an alignment of the outer planets, that only happens every 175 years, for a grand tour of the solar system. Today both Voyager spacecraft continue sending valuable science from the far reaches of our solar system and have officially exited the solar system to reach interstellar space. Along their journey through the solar system, the twin spacecraft revealed details about Jupiter, Saturn, Uranus and Neptune. The gravity of each planet was used to send them on to the next destination. Voyager paved the way for such ambitious orbiter missions as Galileo to Jupiter and Cassini to Saturn. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Future technicians will be needed to help engineer our future on Mars. People with special talents will be in high demand as we prepare for our Journey To Mars. Even simple physical repairs such as fixing an antenna in the extreme environment of Mars will take special skills. Maybe you are the right person for the job of setting up an outpost on the moon Phobos. Are you working on having the right skills? Do you have the desire to dare mighty things? A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Future technicians will be needed to help engineer our future on Mars. People with special talents will be in high demand as we prepare for our Journey To Mars. Even simple physical repairs such as fixing an antenna in the extreme environment of Mars will take special skills. Maybe you are the right person for the job of setting up an outpost on the moon Phobos. Are you working on having the right skills? Do you have the desire to dare mighty things? A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Future technicians will be needed to help engineer our future on Mars. People with special talents will be in high demand as we prepare for our Journey To Mars. Even simple physical repairs such as fixing an antenna in the extreme environment of Mars will take special skills. Maybe you are the right person for the job of setting up an outpost on the moon Phobos. Are you working on having the right skills? Do you have the desire to dare mighty things? A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Future technicians will be needed to help engineer our future on Mars. People with special talents will be in high demand as we prepare for our Journey To Mars. Even simple physical repairs such as fixing an antenna in the extreme environment of Mars will take special skills. Maybe you are the right person for the job of setting up an outpost on the moon Phobos. Are you working on having the right skills? Do you have the desire to dare mighty things? A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Future technicians will be needed to help engineer our future on Mars. People with special talents will be in high demand as we prepare for our Journey To Mars. Even simple physical repairs such as fixing an antenna in the extreme environment of Mars will take special skills. Maybe you are the right person for the job of setting up an outpost on the moon Phobos. Are you working on having the right skills? Do you have the desire to dare mighty things? A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Want to get out of the classroom and be part of the greatest field trip ever? Learning is out of this world! Learning new things can take you places you've never dreamed of, including Mars and its two moons, Phobos and Deimos. No matter where we live, we can always learn something new. Living on Mars means that there will be lots to learn and teachers to teach, but just think of the cool field trips! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Want to get out of the classroom and be part of the greatest field trip ever? Learning is out of this world! Learning new things can take you places you've never dreamed of, including Mars and its two moons, Phobos and Deimos. No matter where we live, we can always learn something new. Living on Mars means that there will be lots to learn and teachers to teach, but just think of the cool field trips! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Want to get out of the classroom and be part of the greatest field trip ever? Learning is out of this world! Learning new things can take you places you've never dreamed of, including Mars and its two moons, Phobos and Deimos. No matter where we live, we can always learn something new. Living on Mars means that there will be lots to learn and teachers to teach, but just think of the cool field trips! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Teach on Mars - NASA Mars Explorers Wanted - Photo Framed - 24x36
Want to get out of the classroom and be part of the greatest field trip ever? Learning is out of this world! Learning new things can take you places you've never dreamed of, including Mars and its two moons, Phobos and Deimos. No matter where we live, we can always learn something new. Living on Mars means that there will be lots to learn and teachers to teach, but just think of the cool field trips! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Teach on Mars - NASA Mars Explorers Wanted - Canvas - 24x36
Want to get out of the classroom and be part of the greatest field trip ever? Learning is out of this world! Learning new things can take you places you've never dreamed of, including Mars and its two moons, Phobos and Deimos. No matter where we live, we can always learn something new. Living on Mars means that there will be lots to learn and teachers to teach, but just think of the cool field trips! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Matte Paper - 12x18
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Matte Paper - 24x36
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Matte Framed - 12x18
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Matte Framed - 24x36
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Photo Paper - 12x18
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Photo Paper - 24x36
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Photo Framed - 12x18
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Photo Framed - 24x36
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Surveyors Wanted - NASA Mars Explorers Wanted - Canvas - 24x36
Surveyors will map and explore Mars and its moons. If you have ever asked the question, What is out there?", maybe this is the job for you! Curiosity leads us to explore new places like Mars and its moons, Phobos and Deimos. What lies beyond the next valley, canyon, crater, or hill is something NASA is working to discover with rovers and with humans someday too. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Star-birthing Region in the Orion Nebula - Matte Paper - 8x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1010
Star-birthing Region in the Orion Nebula - Matte Paper - 10x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1212
Star-birthing Region in the Orion Nebula - Matte Paper - 12x12
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1216
Star-birthing Region in the Orion Nebula - Matte Paper - 12x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1218
Star-birthing Region in the Orion Nebula - Matte Paper - 12x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1414
Star-birthing Region in the Orion Nebula - Matte Paper - 14x14
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1616
Star-birthing Region in the Orion Nebula - Matte Paper - 16x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1620
Star-birthing Region in the Orion Nebula - Matte Paper - 16x20
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1818
Star-birthing Region in the Orion Nebula - Matte Paper - 18x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP1824
Star-birthing Region in the Orion Nebula - Matte Paper - 18x24
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MP2436
Star-birthing Region in the Orion Nebula - Matte Paper - 24x36
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MF0810
Star-birthing Region in the Orion Nebula - Matte Framed - 8x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01MF1010
Star-birthing Region in the Orion Nebula - Matte Framed - 10x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
42.00
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N1976V01MF1212
Star-birthing Region in the Orion Nebula - Matte Framed - 12x12
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
48.00
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N1976V01MF1216
Star-birthing Region in the Orion Nebula - Matte Framed - 12x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
54.00
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N1976V01MF1218
Star-birthing Region in the Orion Nebula - Matte Framed - 12x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
60.00
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N1976V01MF1414
Star-birthing Region in the Orion Nebula - Matte Framed - 14x14
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
60.00
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N1976V01MF1616
Star-birthing Region in the Orion Nebula - Matte Framed - 16x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
66.00
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N1976V01MF1620
Star-birthing Region in the Orion Nebula - Matte Framed - 16x20
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
72.00
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N1976V01MF1818
Star-birthing Region in the Orion Nebula - Matte Framed - 18x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
72.00
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N1976V01MF1824
Star-birthing Region in the Orion Nebula - Matte Framed - 18x24
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
84.00
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N1976V01MF2436
Star-birthing Region in the Orion Nebula - Matte Framed - 24x36
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
120.00
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N1976V01PP0810
Star-birthing Region in the Orion Nebula - Photo Paper - 8x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
16.00
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N1976V01PP1010
Star-birthing Region in the Orion Nebula - Photo Paper - 10x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
18.00
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N1976V01PP1212
Star-birthing Region in the Orion Nebula - Photo Paper - 12x12
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
20.00
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N1976V01PP1216
Star-birthing Region in the Orion Nebula - Photo Paper - 12x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
22.00
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N1976V01PP1218
Star-birthing Region in the Orion Nebula - Photo Paper - 12x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
24.00
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N1976V01PP1414
Star-birthing Region in the Orion Nebula - Photo Paper - 14x14
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PP1616
Star-birthing Region in the Orion Nebula - Photo Paper - 16x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PP1620
Star-birthing Region in the Orion Nebula - Photo Paper - 16x20
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PP1818
Star-birthing Region in the Orion Nebula - Photo Paper - 18x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PP1824
Star-birthing Region in the Orion Nebula - Photo Paper - 18x24
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
34.00
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N1976V01PP2436
Star-birthing Region in the Orion Nebula - Photo Paper - 24x36
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PF0810
Star-birthing Region in the Orion Nebula - Photo Framed - 8x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
46.00
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N1976V01PF1010
Star-birthing Region in the Orion Nebula - Photo Framed - 10x10
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
52.00
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N1976V01PF1212
Star-birthing Region in the Orion Nebula - Photo Framed - 12x12
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PF1216
Star-birthing Region in the Orion Nebula - Photo Framed - 12x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
64.00
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N1976V01PF1218
Star-birthing Region in the Orion Nebula - Photo Framed - 12x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
70.00
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N1976V01PF1414
Star-birthing Region in the Orion Nebula - Photo Framed - 14x14
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
70.00
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N1976V01PF1616
Star-birthing Region in the Orion Nebula - Photo Framed - 16x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
76.00
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N1976V01PF1620
Star-birthing Region in the Orion Nebula - Photo Framed - 16x20
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
82.00
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N1976V01PF1818
Star-birthing Region in the Orion Nebula - Photo Framed - 18x18
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PF1824
Star-birthing Region in the Orion Nebula - Photo Framed - 18x24
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N1976V01PF2436
Star-birthing Region in the Orion Nebula - Photo Framed - 24x36
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
126.00
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N1976V01CA1212
Star-birthing Region in the Orion Nebula - Canvas - 12x12
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
54.00
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N1976V01CA1216
Star-birthing Region in the Orion Nebula - Canvas - 12x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
56.00
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N1976V01CA1616
Star-birthing Region in the Orion Nebula - Canvas - 16x16
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
58.00
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N1976V01CA1620
Star-birthing Region in the Orion Nebula - Canvas - 16x20
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
60.00
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N1976V01CA1824
Star-birthing Region in the Orion Nebula - Canvas - 18x24
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
70.00
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N1976V01CA2436
Star-birthing Region in the Orion Nebula - Canvas - 24x36
In this tiny section of the huge Orion Nebula, clouds of dust and gas churn out stars. The gasses within the nebula are illuminated and heated by ultraviolet light from four hot, massive stars. The magnificent detail revealed by Hubble shows a turbulent star factory set within a churning maelstrom of flowing, luminescent gas. This 2.5-light-year-wide view is only a small portion of the entire nebula, but it includes a star cluster and almost all of the light from the bright glowing clouds of gas that make up the nebula. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula, M42, NGC 1976 Release Date: Nov 20, 1995 Image Credits: NASA, C.R. O'Dell and S.K. Wong (Rice University)
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N4547V00MP0810
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 8x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1010
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 10x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1212
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 12x12
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1216
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 12x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1218
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 12x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1414
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 14x14
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1616
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 16x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1620
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 16x20
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1818
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 18x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP1824
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 18x24
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MP2436
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Paper - 24x36
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF0810
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 8x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1010
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 10x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1212
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 12x12
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1216
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 12x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1218
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 12x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1414
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 14x14
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1616
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 16x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1620
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 16x20
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1818
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 18x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF1824
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 18x24
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00MF2436
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Matte Framed - 24x36
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP0810
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 8x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1010
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 10x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1212
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 12x12
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1216
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 12x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1218
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 12x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1414
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 14x14
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1616
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 16x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1620
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 16x20
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1818
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 18x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP1824
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 18x24
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PP2436
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Paper - 24x36
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF0810
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 8x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1010
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 10x10
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1212
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 12x12
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1216
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 12x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1218
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 12x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1414
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 14x14
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1616
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 16x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1620
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 16x20
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1818
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 18x18
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF1824
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 18x24
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00PF2436
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Photo Framed - 24x36
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00CA1212
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Canvas - 12x12
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00CA1216
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Canvas - 12x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00CA1616
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Canvas - 16x16
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00CA1620
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Canvas - 16x20
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00CA1824
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Canvas - 18x24
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4547V00CA2436
Spitzer-Hubble-Chandra Image of Pinwheel Galaxy - M101 - Canvas - 24x36
The Pinwheel Galaxy, also known as Messier 101, is a face-on spiral galaxy approximately 22 million light-years away from Earth in the constellation Ursa Major. This is a composite image of the spiral galaxy M101 combining views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. The red colors indicate infrared light, yellow is visible, and blue is X-ray. In many ways it is similar to own Milky Way galaxy but larger. The visible light captured by Hubble shows off the swirls of bright stars and glowing gas that give the galaxy its nickname the Pinwheel Galaxy. In contrast, the infrared-light image from the Spitzer telescope sees deeper into the spiral arms to reveal the glow of dust lanes where dense clouds can collapse to form new stars. Chandra's X-ray picture uncovers high-energy features of the galaxy, like remnants of exploded stars or matter zooming around black holes. The overlap of observations from these three telescopes provides an in-depth view of the galaxy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101, NGC 4547, The Pinwheel Galaxy Release Date: Feb 10, 2009 Image Credits: NASA, ESA, CXC, SSC, and STScI
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N4258V00MP0810
Spiral Galaxy NGC 2841 - Matte Paper - 8x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1010
Spiral Galaxy NGC 2841 - Matte Paper - 10x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1212
Spiral Galaxy NGC 2841 - Matte Paper - 12x12
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1216
Spiral Galaxy NGC 2841 - Matte Paper - 12x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1218
Spiral Galaxy NGC 2841 - Matte Paper - 12x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1414
Spiral Galaxy NGC 2841 - Matte Paper - 14x14
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1616
Spiral Galaxy NGC 2841 - Matte Paper - 16x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1620
Spiral Galaxy NGC 2841 - Matte Paper - 16x20
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1818
Spiral Galaxy NGC 2841 - Matte Paper - 18x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP1824
Spiral Galaxy NGC 2841 - Matte Paper - 18x24
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MP2436
Spiral Galaxy NGC 2841 - Matte Paper - 24x36
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MF0810
Spiral Galaxy NGC 2841 - Matte Framed - 8x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
36.00
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N4258V00MF1010
Spiral Galaxy NGC 2841 - Matte Framed - 10x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00MF1212
Spiral Galaxy NGC 2841 - Matte Framed - 12x12
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
48.00
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N4258V00MF1216
Spiral Galaxy NGC 2841 - Matte Framed - 12x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
54.00
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N4258V00MF1218
Spiral Galaxy NGC 2841 - Matte Framed - 12x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
60.00
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N4258V00MF1414
Spiral Galaxy NGC 2841 - Matte Framed - 14x14
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
60.00
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N4258V00MF1616
Spiral Galaxy NGC 2841 - Matte Framed - 16x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
66.00
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N4258V00MF1620
Spiral Galaxy NGC 2841 - Matte Framed - 16x20
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
72.00
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N4258V00MF1818
Spiral Galaxy NGC 2841 - Matte Framed - 18x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
72.00
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N4258V00MF1824
Spiral Galaxy NGC 2841 - Matte Framed - 18x24
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
84.00
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N4258V00MF2436
Spiral Galaxy NGC 2841 - Matte Framed - 24x36
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
120.00
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N4258V00PP0810
Spiral Galaxy NGC 2841 - Photo Paper - 8x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
16.00
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N4258V00PP1010
Spiral Galaxy NGC 2841 - Photo Paper - 10x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
18.00
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N4258V00PP1212
Spiral Galaxy NGC 2841 - Photo Paper - 12x12
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
20.00
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N4258V00PP1216
Spiral Galaxy NGC 2841 - Photo Paper - 12x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
22.00
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N4258V00PP1218
Spiral Galaxy NGC 2841 - Photo Paper - 12x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
24.00
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N4258V00PP1414
Spiral Galaxy NGC 2841 - Photo Paper - 14x14
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00PP1616
Spiral Galaxy NGC 2841 - Photo Paper - 16x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00PP1620
Spiral Galaxy NGC 2841 - Photo Paper - 16x20
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00PP1818
Spiral Galaxy NGC 2841 - Photo Paper - 18x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00PP1824
Spiral Galaxy NGC 2841 - Photo Paper - 18x24
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00PP2436
Spiral Galaxy NGC 2841 - Photo Paper - 24x36
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00PF0810
Spiral Galaxy NGC 2841 - Photo Framed - 8x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
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N4258V00PF1010
Spiral Galaxy NGC 2841 - Photo Framed - 10x10
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
52.00
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N4258V00PF1212
Spiral Galaxy NGC 2841 - Photo Framed - 12x12
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
58.00
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N4258V00PF1216
Spiral Galaxy NGC 2841 - Photo Framed - 12x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
64.00
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N4258V00PF1218
Spiral Galaxy NGC 2841 - Photo Framed - 12x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
70.00
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N4258V00PF1414
Spiral Galaxy NGC 2841 - Photo Framed - 14x14
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
70.00
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N4258V00PF1616
Spiral Galaxy NGC 2841 - Photo Framed - 16x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
76.00
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N4258V00PF1620
Spiral Galaxy NGC 2841 - Photo Framed - 16x20
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
82.00
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N4258V00PF1818
Spiral Galaxy NGC 2841 - Photo Framed - 18x18
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
82.00
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N4258V00PF1824
Spiral Galaxy NGC 2841 - Photo Framed - 18x24
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
100.00
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N4258V00PF2436
Spiral Galaxy NGC 2841 - Photo Framed - 24x36
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
126.00
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N4258V00CA1212
Spiral Galaxy NGC 2841 - Canvas - 12x12
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
54.00
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N4258V00CA1216
Spiral Galaxy NGC 2841 - Canvas - 12x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
56.00
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N4258V00CA1616
Spiral Galaxy NGC 2841 - Canvas - 16x16
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
58.00
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N4258V00CA1620
Spiral Galaxy NGC 2841 - Canvas - 16x20
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
60.00
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N4258V00CA1824
Spiral Galaxy NGC 2841 - Canvas - 18x24
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
70.00
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N4258V00CA2436
Spiral Galaxy NGC 2841 - Canvas - 24x36
This is an example of the prototypical flocculent spiral galaxy with patchy and discontinuous arms. Flocculent means "fluffy" and galaxies like this are patchy without distinct spiral arms. Approximately 30% of known galaxies have these characteristics. Spiral galaxy NGC 2841 lies 46 million light-years away from Earth, in the constellation of Ursa Major, and reveals a majestic disk of stars and dust lanes. It contains a prominent inner ring structure and is home to a large population of young blue stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 2841 Release Date: Sep 22, 2011 Image Credits: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
100.00
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N1309V00MP0810
Spiral Galaxy NGC 1309 - Matte Paper - 8x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
12.00
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N1309V00MP1010
Spiral Galaxy NGC 1309 - Matte Paper - 10x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
14.00
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N1309V00MP1212
Spiral Galaxy NGC 1309 - Matte Paper - 12x12
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
16.00
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N1309V00MP1216
Spiral Galaxy NGC 1309 - Matte Paper - 12x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
18.00
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N1309V00MP1218
Spiral Galaxy NGC 1309 - Matte Paper - 12x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
20.00
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N1309V00MP1414
Spiral Galaxy NGC 1309 - Matte Paper - 14x14
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
20.00
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N1309V00MP1616
Spiral Galaxy NGC 1309 - Matte Paper - 16x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
22.00
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N1309V00MP1620
Spiral Galaxy NGC 1309 - Matte Paper - 16x20
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N1309V00MP1818
Spiral Galaxy NGC 1309 - Matte Paper - 18x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N1309V00MP1824
Spiral Galaxy NGC 1309 - Matte Paper - 18x24
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
28.00
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N1309V00MP2436
Spiral Galaxy NGC 1309 - Matte Paper - 24x36
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
36.00
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N1309V00MF0810
Spiral Galaxy NGC 1309 - Matte Framed - 8x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
36.00
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N1309V00MF1010
Spiral Galaxy NGC 1309 - Matte Framed - 10x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
42.00
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N1309V00MF1212
Spiral Galaxy NGC 1309 - Matte Framed - 12x12
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
48.00
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N1309V00MF1216
Spiral Galaxy NGC 1309 - Matte Framed - 12x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
54.00
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N1309V00MF1218
Spiral Galaxy NGC 1309 - Matte Framed - 12x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
60.00
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N1309V00MF1414
Spiral Galaxy NGC 1309 - Matte Framed - 14x14
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
60.00
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N1309V00MF1616
Spiral Galaxy NGC 1309 - Matte Framed - 16x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
66.00
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N1309V00MF1620
Spiral Galaxy NGC 1309 - Matte Framed - 16x20
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
72.00
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N1309V00MF1818
Spiral Galaxy NGC 1309 - Matte Framed - 18x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
72.00
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N1309V00MF1824
Spiral Galaxy NGC 1309 - Matte Framed - 18x24
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
84.00
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N1309V00MF2436
Spiral Galaxy NGC 1309 - Matte Framed - 24x36
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
120.00
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N1309V00PP0810
Spiral Galaxy NGC 1309 - Photo Paper - 8x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
16.00
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N1309V00PP1010
Spiral Galaxy NGC 1309 - Photo Paper - 10x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
18.00
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N1309V00PP1212
Spiral Galaxy NGC 1309 - Photo Paper - 12x12
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
20.00
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N1309V00PP1216
Spiral Galaxy NGC 1309 - Photo Paper - 12x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
22.00
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N1309V00PP1218
Spiral Galaxy NGC 1309 - Photo Paper - 12x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N1309V00PP1414
Spiral Galaxy NGC 1309 - Photo Paper - 14x14
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N1309V00PP1616
Spiral Galaxy NGC 1309 - Photo Paper - 16x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
26.00
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N1309V00PP1620
Spiral Galaxy NGC 1309 - Photo Paper - 16x20
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
28.00
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N1309V00PP1818
Spiral Galaxy NGC 1309 - Photo Paper - 18x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
28.00
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N1309V00PP1824
Spiral Galaxy NGC 1309 - Photo Paper - 18x24
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PP2436
Spiral Galaxy NGC 1309 - Photo Paper - 24x36
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PF0810
Spiral Galaxy NGC 1309 - Photo Framed - 8x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PF1010
Spiral Galaxy NGC 1309 - Photo Framed - 10x10
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PF1212
Spiral Galaxy NGC 1309 - Photo Framed - 12x12
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
58.00
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N1309V00PF1216
Spiral Galaxy NGC 1309 - Photo Framed - 12x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
64.00
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N1309V00PF1218
Spiral Galaxy NGC 1309 - Photo Framed - 12x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
70.00
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N1309V00PF1414
Spiral Galaxy NGC 1309 - Photo Framed - 14x14
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PF1616
Spiral Galaxy NGC 1309 - Photo Framed - 16x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
76.00
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N1309V00PF1620
Spiral Galaxy NGC 1309 - Photo Framed - 16x20
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PF1818
Spiral Galaxy NGC 1309 - Photo Framed - 18x18
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PF1824
Spiral Galaxy NGC 1309 - Photo Framed - 18x24
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00PF2436
Spiral Galaxy NGC 1309 - Photo Framed - 24x36
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
126.00
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N1309V00CA1212
Spiral Galaxy NGC 1309 - Canvas - 12x12
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
54.00
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N1309V00CA1216
Spiral Galaxy NGC 1309 - Canvas - 12x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
56.00
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N1309V00CA1616
Spiral Galaxy NGC 1309 - Canvas - 16x16
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00CA1620
Spiral Galaxy NGC 1309 - Canvas - 16x20
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00CA1824
Spiral Galaxy NGC 1309 - Canvas - 18x24
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N1309V00CA2436
Spiral Galaxy NGC 1309 - Canvas - 24x36
This pinwheel-shaped spiral galaxy was home to a supernova whose light reached Earth in 2002. Stunning details of the face-on spiral galaxy, are captured in this color image. Scientists are using the supernova burst, SN 2002fk, which took place in NGC 1309 to measure the expansion rate of the universe. Light from this explosion reached Earth in September 2002 and NGC 1309 lies 100 million light-years (30 Megaparsecs) from Earth. It is one of approximately 200 galaxies that make up the Eridanus group of galaxies. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 1309 Release Date: Feb 7, 2006 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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REW07V00MP1218
Some User Assembly Required - NASA Mars Explorers Wanted - Matte Paper - 12x18
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00MP2436
Some User Assembly Required - NASA Mars Explorers Wanted - Matte Paper - 24x36
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00MF1218
Some User Assembly Required - NASA Mars Explorers Wanted - Matte Framed - 12x18
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00MF2436
Some User Assembly Required - NASA Mars Explorers Wanted - Matte Framed - 24x36
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00PP1218
Some User Assembly Required - NASA Mars Explorers Wanted - Photo Paper - 12x18
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00PP2436
Some User Assembly Required - NASA Mars Explorers Wanted - Photo Paper - 24x36
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00PF1218
Some User Assembly Required - NASA Mars Explorers Wanted - Photo Framed - 12x18
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00PF2436
Some User Assembly Required - NASA Mars Explorers Wanted - Photo Framed - 24x36
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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REW07V00CA2436
Some User Assembly Required - NASA Mars Explorers Wanted - Canvas - 24x36
Some assembly will be required to build our future on Mars and its moons. Have you got what it takes to put things together and solve challenges to ensure survival? Dare to forge our future with the latest space-age tools and build spaceships to carry us to Mars and back? Have you got brilliant ideas for creating habitats to protect us and help us grow food or create fuel while we are there? Great! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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N4594V00MP0810
Sombrero Galaxy - M104 - Matte Paper - 8x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1010
Sombrero Galaxy - M104 - Matte Paper - 10x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1212
Sombrero Galaxy - M104 - Matte Paper - 12x12
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1216
Sombrero Galaxy - M104 - Matte Paper - 12x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1218
Sombrero Galaxy - M104 - Matte Paper - 12x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1414
Sombrero Galaxy - M104 - Matte Paper - 14x14
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1616
Sombrero Galaxy - M104 - Matte Paper - 16x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1620
Sombrero Galaxy - M104 - Matte Paper - 16x20
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1818
Sombrero Galaxy - M104 - Matte Paper - 18x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP1824
Sombrero Galaxy - M104 - Matte Paper - 18x24
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MP2436
Sombrero Galaxy - M104 - Matte Paper - 24x36
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF0810
Sombrero Galaxy - M104 - Matte Framed - 8x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1010
Sombrero Galaxy - M104 - Matte Framed - 10x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1212
Sombrero Galaxy - M104 - Matte Framed - 12x12
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1216
Sombrero Galaxy - M104 - Matte Framed - 12x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1218
Sombrero Galaxy - M104 - Matte Framed - 12x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1414
Sombrero Galaxy - M104 - Matte Framed - 14x14
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1616
Sombrero Galaxy - M104 - Matte Framed - 16x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1620
Sombrero Galaxy - M104 - Matte Framed - 16x20
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1818
Sombrero Galaxy - M104 - Matte Framed - 18x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF1824
Sombrero Galaxy - M104 - Matte Framed - 18x24
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00MF2436
Sombrero Galaxy - M104 - Matte Framed - 24x36
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PP0810
Sombrero Galaxy - M104 - Photo Paper - 8x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PP1010
Sombrero Galaxy - M104 - Photo Paper - 10x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
18.00
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N4594V00PP1212
Sombrero Galaxy - M104 - Photo Paper - 12x12
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
20.00
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N4594V00PP1216
Sombrero Galaxy - M104 - Photo Paper - 12x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
22.00
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N4594V00PP1218
Sombrero Galaxy - M104 - Photo Paper - 12x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PP1414
Sombrero Galaxy - M104 - Photo Paper - 14x14
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PP1616
Sombrero Galaxy - M104 - Photo Paper - 16x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
26.00
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N4594V00PP1620
Sombrero Galaxy - M104 - Photo Paper - 16x20
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
28.00
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N4594V00PP1818
Sombrero Galaxy - M104 - Photo Paper - 18x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PP1824
Sombrero Galaxy - M104 - Photo Paper - 18x24
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
34.00
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N4594V00PP2436
Sombrero Galaxy - M104 - Photo Paper - 24x36
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF0810
Sombrero Galaxy - M104 - Photo Framed - 8x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1010
Sombrero Galaxy - M104 - Photo Framed - 10x10
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1212
Sombrero Galaxy - M104 - Photo Framed - 12x12
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1216
Sombrero Galaxy - M104 - Photo Framed - 12x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1218
Sombrero Galaxy - M104 - Photo Framed - 12x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1414
Sombrero Galaxy - M104 - Photo Framed - 14x14
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1616
Sombrero Galaxy - M104 - Photo Framed - 16x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1620
Sombrero Galaxy - M104 - Photo Framed - 16x20
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1818
Sombrero Galaxy - M104 - Photo Framed - 18x18
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF1824
Sombrero Galaxy - M104 - Photo Framed - 18x24
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00PF2436
Sombrero Galaxy - M104 - Photo Framed - 24x36
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
126.00
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N4594V00CA1212
Sombrero Galaxy - M104 - Canvas - 12x12
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00CA1216
Sombrero Galaxy - M104 - Canvas - 12x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00CA1616
Sombrero Galaxy - M104 - Canvas - 16x16
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00CA1620
Sombrero Galaxy - M104 - Canvas - 16x20
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00CA1824
Sombrero Galaxy - M104 - Canvas - 18x24
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N4594V00CA2436
Sombrero Galaxy - M104 - Canvas - 24x36
Thick dust lanes encircle the brilliant white core of this spiral galaxy, seen edge on. The picturesque Sombrero Galaxy lies 28 million light years from Earth in the constellation Virgo. This magnificent galaxy is 50,000 light-years across and has an apparent diameter that is nearly one-fifth the diameter of the full moon, a swarm of stars in a pancake-shaped disk with a glowing central halo of stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Sombrero Galaxy, M104, NGC 4594 Release Date: Oct 2, 2003 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
100.00
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N3370V00MP0810
Silverado Galaxy - NGC 3370 - Matte Paper - 8x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
12.00
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N3370V00MP1010
Silverado Galaxy - NGC 3370 - Matte Paper - 10x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
14.00
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N3370V00MP1212
Silverado Galaxy - NGC 3370 - Matte Paper - 12x12
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
16.00
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N3370V00MP1216
Silverado Galaxy - NGC 3370 - Matte Paper - 12x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
18.00
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N3370V00MP1218
Silverado Galaxy - NGC 3370 - Matte Paper - 12x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
20.00
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N3370V00MP1414
Silverado Galaxy - NGC 3370 - Matte Paper - 14x14
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
20.00
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N3370V00MP1616
Silverado Galaxy - NGC 3370 - Matte Paper - 16x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
22.00
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N3370V00MP1620
Silverado Galaxy - NGC 3370 - Matte Paper - 16x20
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N3370V00MP1818
Silverado Galaxy - NGC 3370 - Matte Paper - 18x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N3370V00MP1824
Silverado Galaxy - NGC 3370 - Matte Paper - 18x24
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
28.00
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N3370V00MP2436
Silverado Galaxy - NGC 3370 - Matte Paper - 24x36
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
36.00
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N3370V00MF0810
Silverado Galaxy - NGC 3370 - Matte Framed - 8x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
36.00
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N3370V00MF1010
Silverado Galaxy - NGC 3370 - Matte Framed - 10x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
42.00
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N3370V00MF1212
Silverado Galaxy - NGC 3370 - Matte Framed - 12x12
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
48.00
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N3370V00MF1216
Silverado Galaxy - NGC 3370 - Matte Framed - 12x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
54.00
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N3370V00MF1218
Silverado Galaxy - NGC 3370 - Matte Framed - 12x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
60.00
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N3370V00MF1414
Silverado Galaxy - NGC 3370 - Matte Framed - 14x14
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
60.00
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N3370V00MF1616
Silverado Galaxy - NGC 3370 - Matte Framed - 16x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
66.00
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N3370V00MF1620
Silverado Galaxy - NGC 3370 - Matte Framed - 16x20
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
72.00
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N3370V00MF1818
Silverado Galaxy - NGC 3370 - Matte Framed - 18x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
72.00
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N3370V00MF1824
Silverado Galaxy - NGC 3370 - Matte Framed - 18x24
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
84.00
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N3370V00MF2436
Silverado Galaxy - NGC 3370 - Matte Framed - 24x36
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
120.00
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N3370V00PP0810
Silverado Galaxy - NGC 3370 - Photo Paper - 8x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
16.00
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N3370V00PP1010
Silverado Galaxy - NGC 3370 - Photo Paper - 10x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
18.00
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N3370V00PP1212
Silverado Galaxy - NGC 3370 - Photo Paper - 12x12
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N3370V00PP1216
Silverado Galaxy - NGC 3370 - Photo Paper - 12x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
22.00
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N3370V00PP1218
Silverado Galaxy - NGC 3370 - Photo Paper - 12x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N3370V00PP1414
Silverado Galaxy - NGC 3370 - Photo Paper - 14x14
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
24.00
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N3370V00PP1616
Silverado Galaxy - NGC 3370 - Photo Paper - 16x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N3370V00PP1620
Silverado Galaxy - NGC 3370 - Photo Paper - 16x20
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
28.00
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N3370V00PP1818
Silverado Galaxy - NGC 3370 - Photo Paper - 18x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
28.00
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N3370V00PP1824
Silverado Galaxy - NGC 3370 - Photo Paper - 18x24
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
34.00
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N3370V00PP2436
Silverado Galaxy - NGC 3370 - Photo Paper - 24x36
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
40.00
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N3370V00PF0810
Silverado Galaxy - NGC 3370 - Photo Framed - 8x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
46.00
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N3370V00PF1010
Silverado Galaxy - NGC 3370 - Photo Framed - 10x10
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
52.00
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N3370V00PF1212
Silverado Galaxy - NGC 3370 - Photo Framed - 12x12
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
58.00
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N3370V00PF1216
Silverado Galaxy - NGC 3370 - Photo Framed - 12x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
64.00
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N3370V00PF1218
Silverado Galaxy - NGC 3370 - Photo Framed - 12x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
70.00
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N3370V00PF1414
Silverado Galaxy - NGC 3370 - Photo Framed - 14x14
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
70.00
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N3370V00PF1616
Silverado Galaxy - NGC 3370 - Photo Framed - 16x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
76.00
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N3370V00PF1620
Silverado Galaxy - NGC 3370 - Photo Framed - 16x20
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N3370V00PF1818
Silverado Galaxy - NGC 3370 - Photo Framed - 18x18
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N3370V00PF1824
Silverado Galaxy - NGC 3370 - Photo Framed - 18x24
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N3370V00PF2436
Silverado Galaxy - NGC 3370 - Photo Framed - 24x36
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
126.00
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N3370V00CA1212
Silverado Galaxy - NGC 3370 - Canvas - 12x12
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
54.00
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N3370V00CA1216
Silverado Galaxy - NGC 3370 - Canvas - 12x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
56.00
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N3370V00CA1616
Silverado Galaxy - NGC 3370 - Canvas - 16x16
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
58.00
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N3370V00CA1620
Silverado Galaxy - NGC 3370 - Canvas - 16x20
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
60.00
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N3370V00CA1824
Silverado Galaxy - NGC 3370 - Canvas - 18x24
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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N3370V00CA2436
Silverado Galaxy - NGC 3370 - Canvas - 24x36
The Silverado Galaxy was home to a supernova that appeared in 1994. The intricate spiral arms of this dusty galaxy contain hot areas of new star formation about 98 million light-years away in the constellation Leo. It is similar to our own Milky Way galaxy in both mass and diameter. NGC 3370 became the first spiral galaxy known to be producing a giant radio-emitting jet. Scientists had previously only observed these giant jets of subatomic particles moving at nearly the speed of light from elliptical galaxies or galaxies in the process of merging. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: NGC 3370, UGC 5887 or Silverado Galaxy Release Date: Sep 4, 2003 Image Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and A. Riess (STScI)
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A12966V00MP0810
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 8x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MP1010
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 10x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MP1212
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 12x12
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MP1216
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 12x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
18.00
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A12966V00MP1218
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 12x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
20.00
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A12966V00MP1414
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 14x14
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MP1616
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 16x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
22.00
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A12966V00MP1620
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 16x20
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
24.00
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A12966V00MP1818
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 18x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
24.00
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A12966V00MP1824
Prehistoric Black Hole (Artist's Concept) - Matte Paper - 18x24
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
28.00
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A12966V00MF0810
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 8x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MF1010
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 10x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
42.00
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A12966V00MF1212
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 12x12
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
48.00
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A12966V00MF1216
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 12x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
54.00
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A12966V00MF1218
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 12x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MF1414
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 14x14
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MF1616
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 16x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MF1620
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 16x20
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MF1818
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 18x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00MF1824
Prehistoric Black Hole (Artist's Concept) - Matte Framed - 18x24
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
84.00
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A12966V00PP0810
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 8x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PP1010
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 10x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PP1212
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 12x12
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
20.00
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A12966V00PP1216
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 12x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
22.00
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A12966V00PP1218
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 12x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
24.00
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A12966V00PP1414
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 14x14
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
24.00
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A12966V00PP1616
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 16x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
26.00
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A12966V00PP1620
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 16x20
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
28.00
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A12966V00PP1818
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 18x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PP1824
Prehistoric Black Hole (Artist's Concept) - Photo Paper - 18x24
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
34.00
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A12966V00PF0810
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 8x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
46.00
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A12966V00PF1010
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 10x10
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
52.00
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A12966V00PF1212
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 12x12
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PF1216
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 12x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
64.00
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A12966V00PF1218
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 12x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PF1414
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 14x14
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PF1616
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 16x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
76.00
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A12966V00PF1620
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 16x20
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PF1818
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 18x18
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00PF1824
Prehistoric Black Hole (Artist's Concept) - Photo Framed - 18x24
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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A12966V00CA1212
Prehistoric Black Hole (Artist's Concept) - Canvas - 12x12
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
54.00
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A12966V00CA1216
Prehistoric Black Hole (Artist's Concept) - Canvas - 12x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
56.00
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A12966V00CA1616
Prehistoric Black Hole (Artist's Concept) - Canvas - 16x16
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
58.00
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A12966V00CA1620
Prehistoric Black Hole (Artist's Concept) - Canvas - 16x20
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
60.00
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A12966V00CA1824
Prehistoric Black Hole (Artist's Concept) - Canvas - 18x24
This artist's conception illustrates one of the most primitive supermassive black holes known at the core of a young, star-rich galaxy. Astronomers have uncovered two of these early objects, dating back to about 13 billion years ago. These monstrous black holes are among the most distant known. They appear to be in the very earliest stages of formation, earlier than any observed so far, because they lack dust. Usually, the accretion disk of a black hole becomes surrounded by a dark, dusty structure called a dust torus. But for the primitive black holes, this dust is missing and only gas disks are observed. This is because the early universe was surprisingly clean. Not enough time had passed for molecules to clump together into dust particles, so some black holes forming in this era started out lacking dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Image Credits: NASA/JPL-Caltech
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N5457V00MP0810
Pinwheel Galaxy - M101 - Matte Paper - 8x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
12.00
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N5457V00MP1010
Pinwheel Galaxy - M101 - Matte Paper - 10x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
14.00
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N5457V00MP1212
Pinwheel Galaxy - M101 - Matte Paper - 12x12
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
16.00
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N5457V00MP1216
Pinwheel Galaxy - M101 - Matte Paper - 12x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
18.00
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N5457V00MP1218
Pinwheel Galaxy - M101 - Matte Paper - 12x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
20.00
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N5457V00MP1414
Pinwheel Galaxy - M101 - Matte Paper - 14x14
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
20.00
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N5457V00MP1616
Pinwheel Galaxy - M101 - Matte Paper - 16x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
22.00
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N5457V00MP1620
Pinwheel Galaxy - M101 - Matte Paper - 16x20
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
24.00
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N5457V00MP1818
Pinwheel Galaxy - M101 - Matte Paper - 18x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
24.00
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N5457V00MP1824
Pinwheel Galaxy - M101 - Matte Paper - 18x24
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
28.00
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N5457V00MP2436
Pinwheel Galaxy - M101 - Matte Paper - 24x36
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
36.00
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N5457V00MF0810
Pinwheel Galaxy - M101 - Matte Framed - 8x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
36.00
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N5457V00MF1010
Pinwheel Galaxy - M101 - Matte Framed - 10x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
42.00
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N5457V00MF1212
Pinwheel Galaxy - M101 - Matte Framed - 12x12
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
48.00
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N5457V00MF1216
Pinwheel Galaxy - M101 - Matte Framed - 12x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
54.00
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N5457V00MF1218
Pinwheel Galaxy - M101 - Matte Framed - 12x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
60.00
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N5457V00MF1414
Pinwheel Galaxy - M101 - Matte Framed - 14x14
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
60.00
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N5457V00MF1616
Pinwheel Galaxy - M101 - Matte Framed - 16x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
66.00
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N5457V00MF1620
Pinwheel Galaxy - M101 - Matte Framed - 16x20
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
72.00
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N5457V00MF1818
Pinwheel Galaxy - M101 - Matte Framed - 18x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
72.00
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N5457V00MF1824
Pinwheel Galaxy - M101 - Matte Framed - 18x24
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
84.00
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N5457V00MF2436
Pinwheel Galaxy - M101 - Matte Framed - 24x36
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
120.00
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N5457V00PP0810
Pinwheel Galaxy - M101 - Photo Paper - 8x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
16.00
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N5457V00PP1010
Pinwheel Galaxy - M101 - Photo Paper - 10x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
18.00
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N5457V00PP1212
Pinwheel Galaxy - M101 - Photo Paper - 12x12
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
20.00
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N5457V00PP1216
Pinwheel Galaxy - M101 - Photo Paper - 12x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
22.00
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N5457V00PP1218
Pinwheel Galaxy - M101 - Photo Paper - 12x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
24.00
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N5457V00PP1414
Pinwheel Galaxy - M101 - Photo Paper - 14x14
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
24.00
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N5457V00PP1616
Pinwheel Galaxy - M101 - Photo Paper - 16x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
26.00
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N5457V00PP1620
Pinwheel Galaxy - M101 - Photo Paper - 16x20
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
28.00
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N5457V00PP1818
Pinwheel Galaxy - M101 - Photo Paper - 18x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
28.00
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N5457V00PP1824
Pinwheel Galaxy - M101 - Photo Paper - 18x24
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
34.00
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N5457V00PP2436
Pinwheel Galaxy - M101 - Photo Paper - 24x36
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
40.00
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N5457V00PF0810
Pinwheel Galaxy - M101 - Photo Framed - 8x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
46.00
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N5457V00PF1010
Pinwheel Galaxy - M101 - Photo Framed - 10x10
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
52.00
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N5457V00PF1212
Pinwheel Galaxy - M101 - Photo Framed - 12x12
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
58.00
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N5457V00PF1216
Pinwheel Galaxy - M101 - Photo Framed - 12x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
64.00
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N5457V00PF1218
Pinwheel Galaxy - M101 - Photo Framed - 12x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
70.00
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N5457V00PF1414
Pinwheel Galaxy - M101 - Photo Framed - 14x14
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
70.00
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N5457V00PF1616
Pinwheel Galaxy - M101 - Photo Framed - 16x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
76.00
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N5457V00PF1620
Pinwheel Galaxy - M101 - Photo Framed - 16x20
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
82.00
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N5457V00PF1818
Pinwheel Galaxy - M101 - Photo Framed - 18x18
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
82.00
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N5457V00PF1824
Pinwheel Galaxy - M101 - Photo Framed - 18x24
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
100.00
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N5457V00PF2436
Pinwheel Galaxy - M101 - Photo Framed - 24x36
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
126.00
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N5457V00CA1212
Pinwheel Galaxy - M101 - Canvas - 12x12
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
54.00
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N5457V00CA1216
Pinwheel Galaxy - M101 - Canvas - 12x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
56.00
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N5457V00CA1616
Pinwheel Galaxy - M101 - Canvas - 16x16
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
58.00
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N5457V00CA1620
Pinwheel Galaxy - M101 - Canvas - 16x20
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
60.00
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N5457V00CA1824
Pinwheel Galaxy - M101 - Canvas - 18x24
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
70.00
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N5457V00CA2436
Pinwheel Galaxy - M101 - Canvas - 24x36
M101 lies 21 million light-years distant from Earth in the constellation Ursa Major. This giant spiral disk of stars, dust and gas is 170,000 light-years across, almost twice the diameter of our Milky Way galaxy. Also know as the Pinwheel Galaxy, M101 is estimated to contain at least one trillion stars. This galaxy portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 spanning March 1994, September 1994, June 1999, November 2002, and January 2003. It was first discovered by Pierre Méchain on March 27, 1781, and Charles Messier verified its position for inclusion as one of the final entries in the Messier Catalogue. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M101 (NGC 5457, Pinwheel Galaxy) Release Date: Feb 28, 2006 Image Credits: Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI; Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum; Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
100.00
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RSX02V00MP1218
Phobos & Deimos - SpaceX Mars Travel - Matte Paper - 12x18
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX02V00MP2436
Phobos & Deimos - SpaceX Mars Travel - Matte Paper - 24x36
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX02V00MF1218
Phobos & Deimos - SpaceX Mars Travel - Matte Framed - 12x18
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX02V00MF2436
Phobos & Deimos - SpaceX Mars Travel - Matte Framed - 24x36
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX02V00PP1218
Phobos & Deimos - SpaceX Mars Travel - Photo Paper - 12x18
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
24.00
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RSX02V00PP2436
Phobos & Deimos - SpaceX Mars Travel - Photo Paper - 24x36
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX02V00PF1218
Phobos & Deimos - SpaceX Mars Travel - Photo Framed - 12x18
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
70.00
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RSX02V00PF2436
Phobos & Deimos - SpaceX Mars Travel - Photo Framed - 24x36
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
126.00
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RSX02V00CA2436
Phobos & Deimos - SpaceX Mars Travel - Canvas - 24x36
The twin moons of Mars are calling. Plan your vacation to Phobos and Deimos! Come take a stroll, but be careful. Gravity on both of these very small moons is very weak. Standing on Phobos you will be 1000 times lighter than on Earth. One big jump and you might accidentally fly off into space! A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
100.00
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N1976V00MP0810
Orion Nebula - M42 - Matte Paper - 8x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
12.00
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N1976V00MP1010
Orion Nebula - M42 - Matte Paper - 10x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00MP1212
Orion Nebula - M42 - Matte Paper - 12x12
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
16.00
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N1976V00MP1216
Orion Nebula - M42 - Matte Paper - 12x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
18.00
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N1976V00MP1218
Orion Nebula - M42 - Matte Paper - 12x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
20.00
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N1976V00MP1414
Orion Nebula - M42 - Matte Paper - 14x14
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
20.00
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N1976V00MP1616
Orion Nebula - M42 - Matte Paper - 16x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
22.00
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N1976V00MP1620
Orion Nebula - M42 - Matte Paper - 16x20
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
24.00
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N1976V00MP1818
Orion Nebula - M42 - Matte Paper - 18x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
24.00
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N1976V00MP1824
Orion Nebula - M42 - Matte Paper - 18x24
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
28.00
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N1976V00MP2436
Orion Nebula - M42 - Matte Paper - 24x36
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
36.00
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N1976V00MF0810
Orion Nebula - M42 - Matte Framed - 8x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
36.00
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N1976V00MF1010
Orion Nebula - M42 - Matte Framed - 10x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
42.00
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N1976V00MF1212
Orion Nebula - M42 - Matte Framed - 12x12
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
48.00
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N1976V00MF1216
Orion Nebula - M42 - Matte Framed - 12x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
54.00
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N1976V00MF1218
Orion Nebula - M42 - Matte Framed - 12x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00MF1414
Orion Nebula - M42 - Matte Framed - 14x14
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
60.00
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N1976V00MF1616
Orion Nebula - M42 - Matte Framed - 16x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
66.00
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N1976V00MF1620
Orion Nebula - M42 - Matte Framed - 16x20
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
72.00
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N1976V00MF1818
Orion Nebula - M42 - Matte Framed - 18x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
72.00
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N1976V00MF1824
Orion Nebula - M42 - Matte Framed - 18x24
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
84.00
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N1976V00MF2436
Orion Nebula - M42 - Matte Framed - 24x36
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
120.00
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N1976V00PP0810
Orion Nebula - M42 - Photo Paper - 8x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
16.00
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N1976V00PP1010
Orion Nebula - M42 - Photo Paper - 10x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
18.00
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N1976V00PP1212
Orion Nebula - M42 - Photo Paper - 12x12
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00PP1216
Orion Nebula - M42 - Photo Paper - 12x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
22.00
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N1976V00PP1218
Orion Nebula - M42 - Photo Paper - 12x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
24.00
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N1976V00PP1414
Orion Nebula - M42 - Photo Paper - 14x14
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
24.00
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N1976V00PP1616
Orion Nebula - M42 - Photo Paper - 16x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
26.00
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N1976V00PP1620
Orion Nebula - M42 - Photo Paper - 16x20
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
28.00
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N1976V00PP1818
Orion Nebula - M42 - Photo Paper - 18x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
28.00
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N1976V00PP1824
Orion Nebula - M42 - Photo Paper - 18x24
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
34.00
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N1976V00PP2436
Orion Nebula - M42 - Photo Paper - 24x36
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00PF0810
Orion Nebula - M42 - Photo Framed - 8x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
46.00
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N1976V00PF1010
Orion Nebula - M42 - Photo Framed - 10x10
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
52.00
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N1976V00PF1212
Orion Nebula - M42 - Photo Framed - 12x12
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
58.00
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N1976V00PF1216
Orion Nebula - M42 - Photo Framed - 12x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
64.00
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N1976V00PF1218
Orion Nebula - M42 - Photo Framed - 12x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00PF1414
Orion Nebula - M42 - Photo Framed - 14x14
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00PF1616
Orion Nebula - M42 - Photo Framed - 16x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
76.00
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N1976V00PF1620
Orion Nebula - M42 - Photo Framed - 16x20
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00PF1818
Orion Nebula - M42 - Photo Framed - 18x18
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00PF1824
Orion Nebula - M42 - Photo Framed - 18x24
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00PF2436
Orion Nebula - M42 - Photo Framed - 24x36
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
126.00
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N1976V00CA1212
Orion Nebula - M42 - Canvas - 12x12
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00CA1216
Orion Nebula - M42 - Canvas - 12x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00CA1616
Orion Nebula - M42 - Canvas - 16x16
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00CA1620
Orion Nebula - M42 - Canvas - 16x20
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00CA1824
Orion Nebula - M42 - Canvas - 18x24
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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N1976V00CA2436
Orion Nebula - M42 - Canvas - 24x36
The Orion Nebula is a cavern of tumultuous gas and dust where thousands of stars are forming. Energy released by young stars transforms the place where they are born, whipping the surroundings into fantastic forms. This turbulent star formation region is one of the most dramatic and photogenic celestial objects. Over 3,000 stars of different sizes appear in this image. Some of these stars have never been seen in visible light and reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that resemble the Grand Canyon. The Orion Nebula is a vast picture book of star formations, from massive, young stars that are shaping the nebula to pillars of dense gas that can be home to budding stars. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Orion Nebula (M42, NGC 1976) Release Date: Jan 11, 2006 Image Credits: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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RSX03V00MP1218
Olympus Mons - SpaceX Mars Travel - Matte Paper - 12x18
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00MP2436
Olympus Mons - SpaceX Mars Travel - Matte Paper - 24x36
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00MF1218
Olympus Mons - SpaceX Mars Travel - Matte Framed - 12x18
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00MF2436
Olympus Mons - SpaceX Mars Travel - Matte Framed - 24x36
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00PP1218
Olympus Mons - SpaceX Mars Travel - Photo Paper - 12x18
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00PP2436
Olympus Mons - SpaceX Mars Travel - Photo Paper - 24x36
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00PF1218
Olympus Mons - SpaceX Mars Travel - Photo Framed - 12x18
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00PF2436
Olympus Mons - SpaceX Mars Travel - Photo Framed - 24x36
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RSX03V00CA2436
Olympus Mons - SpaceX Mars Travel - Canvas - 24x36
Adventure awaits! Come explore Mars’ ultimate vacation destinations today! Olympus Mons, which means Mount Olympus in Latin, is the largest shield volcano in our solar system. It is an amazing 374 miles in diameter, which is just about the same size as the state of Arizona! It's just so big, it had to be named after the mythical home of the gods of Greek legend. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Like the NASA exoplanet ads before them, the Mars posters released to the public by SpaceX portray an optimistic future in a fun and positive ’50s styleImage Credits: SpaceX
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RVF02V00MP1218
Mars - NASA Visions of the Future - Matte Paper - 12x18
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF02V00MP2436
Mars - NASA Visions of the Future - Matte Paper - 24x36
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF02V00MF1218
Mars - NASA Visions of the Future - Matte Framed - 12x18
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Mars - NASA Visions of the Future - Matte Framed - 24x36
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Mars - NASA Visions of the Future - Photo Paper - 12x18
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Mars - NASA Visions of the Future - Photo Paper - 24x36
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Mars - NASA Visions of the Future - Photo Framed - 12x18
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Mars - NASA Visions of the Future - Photo Framed - 24x36
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Mars - NASA Visions of the Future - Canvas - 24x36
NASA's Mars Exploration Program seeks to understand whether Mars was, is, or can be a habitable world. Missions like Mars Pathfinder, Mars Exploration Rovers, Mars Science Laboratory and Mars Reconnaissance Orbiter, and many others, have provided important information in understanding Mars. This poster imagines a future when we have achieved our vision of human exploration of Mars, taking a nostalgic look back at the great imagined milestones of Mars exploration that will someday be celebrated as “historic sites.” A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Matte Paper - 12x18
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Matte Paper - 24x36
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Matte Framed - 12x18
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Matte Framed - 24x36
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Photo Paper - 12x18
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Photo Paper - 24x36
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Photo Framed - 12x18
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Photo Framed - 24x36
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-186f - NASA Visions of the Future - Canvas - 24x36
Plants might be very different colors on planets around other stars, influenced by a different spectrum of available light from their star. Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star. This means liquid water could exist on the planet's surface, but its star is much cooler and redder than our Sun. If plant life does exist on a planet like Kepler-186f, photosynthesis could have been influenced by the red-wavelength photons of the star, making a color palette that's very different than the greens on Earth. This discovery was made by Kepler, NASA's planet hunting telescope. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Matte Paper - 12x18
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Matte Paper - 24x36
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Matte Framed - 12x18
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Matte Framed - 24x36
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Photo Paper - 12x18
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Photo Paper - 24x36
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Photo Framed - 12x18
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Kepler-16b - NASA Visions of the Future - Photo Framed - 24x36
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF12V00CA2436
Kepler-16b - NASA Visions of the Future - Canvas - 24x36
Like the planet "Tatooine" in Star Wars, Kepler-16b orbits a pair of stars. Shown here as a terrestrial planet, Kepler-16b could also be a gas giant like Saturn. The possibility of life on this unusual world are not good. It has an average temperature of −85 °C, similar to that of dry ice. But the discovery indicates that the double-sunset depicted in the movie is no longer science fiction. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00MP1218
Jupiter - NASA Visions of the Future - Matte Paper - 12x18
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00MP2436
Jupiter - NASA Visions of the Future - Matte Paper - 24x36
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00MF1218
Jupiter - NASA Visions of the Future - Matte Framed - 12x18
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00MF2436
Jupiter - NASA Visions of the Future - Matte Framed - 24x36
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00PP1218
Jupiter - NASA Visions of the Future - Photo Paper - 12x18
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00PP2436
Jupiter - NASA Visions of the Future - Photo Paper - 24x36
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00PF1218
Jupiter - NASA Visions of the Future - Photo Framed - 12x18
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00PF2436
Jupiter - NASA Visions of the Future - Photo Framed - 24x36
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF06V00CA2436
Jupiter - NASA Visions of the Future - Canvas - 24x36
NASA's Juno spacecraft arrived at Jupiter in July of 2016 to observe Jupiter's auroras from above the polar regions, studying them like never before possible. The clouds of Jupiter boast the most spectacular light show in the solar system, with dazzling northern and southern lights to impress any space traveler. Jupiter's auroras are hundreds of times more powerful than the Aurora Borealis on Earth, and they form a glowing ring around each pole that is bigger than our home planet. Revolving outside this Jovian aurora are the glowing, electric “footprints” of Jupiter's three largest moons. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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N7293V00MP0810
Helix Nebula - NGC 7293 - Matte Paper - 8x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MP1010
Helix Nebula - NGC 7293 - Matte Paper - 10x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MP1212
Helix Nebula - NGC 7293 - Matte Paper - 12x12
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MP1216
Helix Nebula - NGC 7293 - Matte Paper - 12x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MP1218
Helix Nebula - NGC 7293 - Matte Paper - 12x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MP1414
Helix Nebula - NGC 7293 - Matte Paper - 14x14
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MP1616
Helix Nebula - NGC 7293 - Matte Paper - 16x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MP1620
Helix Nebula - NGC 7293 - Matte Paper - 16x20
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
24.00
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N7293V00MP1818
Helix Nebula - NGC 7293 - Matte Paper - 18x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
24.00
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N7293V00MP1824
Helix Nebula - NGC 7293 - Matte Paper - 18x24
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
28.00
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N7293V00MP2436
Helix Nebula - NGC 7293 - Matte Paper - 24x36
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
36.00
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N7293V00MF0810
Helix Nebula - NGC 7293 - Matte Framed - 8x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
36.00
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N7293V00MF1010
Helix Nebula - NGC 7293 - Matte Framed - 10x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
42.00
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N7293V00MF1212
Helix Nebula - NGC 7293 - Matte Framed - 12x12
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
48.00
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N7293V00MF1216
Helix Nebula - NGC 7293 - Matte Framed - 12x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
54.00
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N7293V00MF1218
Helix Nebula - NGC 7293 - Matte Framed - 12x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
60.00
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N7293V00MF1414
Helix Nebula - NGC 7293 - Matte Framed - 14x14
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
60.00
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N7293V00MF1616
Helix Nebula - NGC 7293 - Matte Framed - 16x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
66.00
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N7293V00MF1620
Helix Nebula - NGC 7293 - Matte Framed - 16x20
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
72.00
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N7293V00MF1818
Helix Nebula - NGC 7293 - Matte Framed - 18x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MF1824
Helix Nebula - NGC 7293 - Matte Framed - 18x24
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00MF2436
Helix Nebula - NGC 7293 - Matte Framed - 24x36
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP0810
Helix Nebula - NGC 7293 - Photo Paper - 8x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
16.00
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N7293V00PP1010
Helix Nebula - NGC 7293 - Photo Paper - 10x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1212
Helix Nebula - NGC 7293 - Photo Paper - 12x12
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1216
Helix Nebula - NGC 7293 - Photo Paper - 12x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1218
Helix Nebula - NGC 7293 - Photo Paper - 12x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1414
Helix Nebula - NGC 7293 - Photo Paper - 14x14
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1616
Helix Nebula - NGC 7293 - Photo Paper - 16x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1620
Helix Nebula - NGC 7293 - Photo Paper - 16x20
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1818
Helix Nebula - NGC 7293 - Photo Paper - 18x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP1824
Helix Nebula - NGC 7293 - Photo Paper - 18x24
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PP2436
Helix Nebula - NGC 7293 - Photo Paper - 24x36
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF0810
Helix Nebula - NGC 7293 - Photo Framed - 8x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF1010
Helix Nebula - NGC 7293 - Photo Framed - 10x10
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF1212
Helix Nebula - NGC 7293 - Photo Framed - 12x12
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF1216
Helix Nebula - NGC 7293 - Photo Framed - 12x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF1218
Helix Nebula - NGC 7293 - Photo Framed - 12x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
70.00
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N7293V00PF1414
Helix Nebula - NGC 7293 - Photo Framed - 14x14
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
70.00
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N7293V00PF1616
Helix Nebula - NGC 7293 - Photo Framed - 16x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
76.00
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N7293V00PF1620
Helix Nebula - NGC 7293 - Photo Framed - 16x20
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF1818
Helix Nebula - NGC 7293 - Photo Framed - 18x18
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF1824
Helix Nebula - NGC 7293 - Photo Framed - 18x24
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00PF2436
Helix Nebula - NGC 7293 - Photo Framed - 24x36
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
126.00
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N7293V00CA1212
Helix Nebula - NGC 7293 - Canvas - 12x12
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00CA1216
Helix Nebula - NGC 7293 - Canvas - 12x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00CA1616
Helix Nebula - NGC 7293 - Canvas - 16x16
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00CA1620
Helix Nebula - NGC 7293 - Canvas - 16x20
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00CA1824
Helix Nebula - NGC 7293 - Canvas - 18x24
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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N7293V00CA2436
Helix Nebula - NGC 7293 - Canvas - 24x36
A cloud of gas is expelled and illuminated by the dying star at the center of the Helix Nebula. Looks can be deceiving when it comes to celestial objects. From the vantage point of Earth the Helix Nebula looks like a donut, but it is actually more complex. Because these objects are so far away, it is difficult to see their three-dimensional structure. The Helix Nebula looks a bit like a doughnut, but earlier images of this gaseous envelope ejected by a dying, sun-like star were interpreted to show that the Helix's form resembled a snake-like coil. Most recently, the Helix's structure has become even more perplexing with evidence suggesting that the Helix consists of two nearly perpendicular discs. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Helix Nebula, NGC 7293 Release Date: Dec 16, 2004 Image Credits: NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI)
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RVF11V00MP1218
HD 40307g - NASA Visions of the Future - Matte Paper - 12x18
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF11V00MP2436
HD 40307g - NASA Visions of the Future - Matte Paper - 24x36
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
36.00
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RVF11V00MF1218
HD 40307g - NASA Visions of the Future - Matte Framed - 12x18
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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https://posternauts.com/cdn/shop/products/mockup-f0e33142_medium.jpg?v=1496443324,
RVF11V00MF2436
HD 40307g - NASA Visions of the Future - Matte Framed - 24x36
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
120.00
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RVF11V00PP1218
HD 40307g - NASA Visions of the Future - Photo Paper - 12x18
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF11V00PP2436
HD 40307g - NASA Visions of the Future - Photo Paper - 24x36
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF11V00PF1218
HD 40307g - NASA Visions of the Future - Photo Framed - 12x18
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF11V00PF2436
HD 40307g - NASA Visions of the Future - Photo Framed - 24x36
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF11V00CA2436
HD 40307g - NASA Visions of the Future - Canvas - 24x36
A super-Earth is a planet with a mass greater than Earth, but still significantly less than the ice giants of our solar system, Uranus and Neptune. What would be the attraction of visiting a super-Earth, a bigger, more massive planet than our own? The easy answer is more gravity! HD 40307g is twice as big in volume as the Earth and and scientists aren't sure if it has a rocky surface or one that's buried beneath thick layers of gas and ice. One thing that is certain though, at eight time the Earth's mass, its gravitational pull is much, much stronger. This poster depicts thrill-seekers taking advantage of these gravitational differences. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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N5139V00MP0810
Globular Star Cluster Omega Centauri - Matte Paper - 8x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1010
Globular Star Cluster Omega Centauri - Matte Paper - 10x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1212
Globular Star Cluster Omega Centauri - Matte Paper - 12x12
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1216
Globular Star Cluster Omega Centauri - Matte Paper - 12x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1218
Globular Star Cluster Omega Centauri - Matte Paper - 12x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1414
Globular Star Cluster Omega Centauri - Matte Paper - 14x14
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1616
Globular Star Cluster Omega Centauri - Matte Paper - 16x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1620
Globular Star Cluster Omega Centauri - Matte Paper - 16x20
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1818
Globular Star Cluster Omega Centauri - Matte Paper - 18x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP1824
Globular Star Cluster Omega Centauri - Matte Paper - 18x24
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MP2436
Globular Star Cluster Omega Centauri - Matte Paper - 24x36
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF0810
Globular Star Cluster Omega Centauri - Matte Framed - 8x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1010
Globular Star Cluster Omega Centauri - Matte Framed - 10x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1212
Globular Star Cluster Omega Centauri - Matte Framed - 12x12
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1216
Globular Star Cluster Omega Centauri - Matte Framed - 12x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1218
Globular Star Cluster Omega Centauri - Matte Framed - 12x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1414
Globular Star Cluster Omega Centauri - Matte Framed - 14x14
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1616
Globular Star Cluster Omega Centauri - Matte Framed - 16x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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Globular Star Cluster Omega Centauri - Matte Framed - 16x20
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1818
Globular Star Cluster Omega Centauri - Matte Framed - 18x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF1824
Globular Star Cluster Omega Centauri - Matte Framed - 18x24
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00MF2436
Globular Star Cluster Omega Centauri - Matte Framed - 24x36
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP0810
Globular Star Cluster Omega Centauri - Photo Paper - 8x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1010
Globular Star Cluster Omega Centauri - Photo Paper - 10x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1212
Globular Star Cluster Omega Centauri - Photo Paper - 12x12
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1216
Globular Star Cluster Omega Centauri - Photo Paper - 12x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1218
Globular Star Cluster Omega Centauri - Photo Paper - 12x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1414
Globular Star Cluster Omega Centauri - Photo Paper - 14x14
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1616
Globular Star Cluster Omega Centauri - Photo Paper - 16x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1620
Globular Star Cluster Omega Centauri - Photo Paper - 16x20
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1818
Globular Star Cluster Omega Centauri - Photo Paper - 18x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP1824
Globular Star Cluster Omega Centauri - Photo Paper - 18x24
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PP2436
Globular Star Cluster Omega Centauri - Photo Paper - 24x36
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF0810
Globular Star Cluster Omega Centauri - Photo Framed - 8x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1010
Globular Star Cluster Omega Centauri - Photo Framed - 10x10
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1212
Globular Star Cluster Omega Centauri - Photo Framed - 12x12
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1216
Globular Star Cluster Omega Centauri - Photo Framed - 12x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1218
Globular Star Cluster Omega Centauri - Photo Framed - 12x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1414
Globular Star Cluster Omega Centauri - Photo Framed - 14x14
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1616
Globular Star Cluster Omega Centauri - Photo Framed - 16x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1620
Globular Star Cluster Omega Centauri - Photo Framed - 16x20
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1818
Globular Star Cluster Omega Centauri - Photo Framed - 18x18
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF1824
Globular Star Cluster Omega Centauri - Photo Framed - 18x24
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00PF2436
Globular Star Cluster Omega Centauri - Photo Framed - 24x36
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00CA1212
Globular Star Cluster Omega Centauri - Canvas - 12x12
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00CA1216
Globular Star Cluster Omega Centauri - Canvas - 12x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00CA1616
Globular Star Cluster Omega Centauri - Canvas - 16x16
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00CA1620
Globular Star Cluster Omega Centauri - Canvas - 16x20
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00CA1824
Globular Star Cluster Omega Centauri - Canvas - 18x24
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N5139V00CA2436
Globular Star Cluster Omega Centauri - Canvas - 24x36
Omega Centauri is one of the biggest star clusters in the Milky Way. This colorful collection of 100,000 stars is from a small region inside the Omega Centauri globular cluster, a dense group of nearly 10 million stars in the constellation of Centaurus. The cluster is 15,800 light-years from Earth and one of the few globular clusters visible to the naked eye. It was first identified as a non-stellar object (not a single star) in 1677, by Edmond Halley, but was observed by man at least as early as 150 A.D. by the Greco-Roman astronomer, Ptolemy. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Omega Centauri, NGC 5139 Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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Globular Cluster 47 Tucanae - Matte Paper - 8x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1010
Globular Cluster 47 Tucanae - Matte Paper - 10x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1212
Globular Cluster 47 Tucanae - Matte Paper - 12x12
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1216
Globular Cluster 47 Tucanae - Matte Paper - 12x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1218
Globular Cluster 47 Tucanae - Matte Paper - 12x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1414
Globular Cluster 47 Tucanae - Matte Paper - 14x14
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1616
Globular Cluster 47 Tucanae - Matte Paper - 16x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1620
Globular Cluster 47 Tucanae - Matte Paper - 16x20
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1818
Globular Cluster 47 Tucanae - Matte Paper - 18x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MP1824
Globular Cluster 47 Tucanae - Matte Paper - 18x24
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF0810
Globular Cluster 47 Tucanae - Matte Framed - 8x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1010
Globular Cluster 47 Tucanae - Matte Framed - 10x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1212
Globular Cluster 47 Tucanae - Matte Framed - 12x12
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1216
Globular Cluster 47 Tucanae - Matte Framed - 12x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1218
Globular Cluster 47 Tucanae - Matte Framed - 12x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1414
Globular Cluster 47 Tucanae - Matte Framed - 14x14
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1616
Globular Cluster 47 Tucanae - Matte Framed - 16x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1620
Globular Cluster 47 Tucanae - Matte Framed - 16x20
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1818
Globular Cluster 47 Tucanae - Matte Framed - 18x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00MF1824
Globular Cluster 47 Tucanae - Matte Framed - 18x24
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PP0810
Globular Cluster 47 Tucanae - Photo Paper - 8x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PP1010
Globular Cluster 47 Tucanae - Photo Paper - 10x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PP1212
Globular Cluster 47 Tucanae - Photo Paper - 12x12
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PP1216
Globular Cluster 47 Tucanae - Photo Paper - 12x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PP1218
Globular Cluster 47 Tucanae - Photo Paper - 12x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PP1414
Globular Cluster 47 Tucanae - Photo Paper - 14x14
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PP1616
Globular Cluster 47 Tucanae - Photo Paper - 16x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
26.00
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N0104V00PP1620
Globular Cluster 47 Tucanae - Photo Paper - 16x20
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
28.00
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N0104V00PP1818
Globular Cluster 47 Tucanae - Photo Paper - 18x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
28.00
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N0104V00PP1824
Globular Cluster 47 Tucanae - Photo Paper - 18x24
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF0810
Globular Cluster 47 Tucanae - Photo Framed - 8x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF1010
Globular Cluster 47 Tucanae - Photo Framed - 10x10
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF1212
Globular Cluster 47 Tucanae - Photo Framed - 12x12
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
58.00
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N0104V00PF1216
Globular Cluster 47 Tucanae - Photo Framed - 12x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
64.00
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N0104V00PF1218
Globular Cluster 47 Tucanae - Photo Framed - 12x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF1414
Globular Cluster 47 Tucanae - Photo Framed - 14x14
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF1616
Globular Cluster 47 Tucanae - Photo Framed - 16x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF1620
Globular Cluster 47 Tucanae - Photo Framed - 16x20
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF1818
Globular Cluster 47 Tucanae - Photo Framed - 18x18
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00PF1824
Globular Cluster 47 Tucanae - Photo Framed - 18x24
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00CA1212
Globular Cluster 47 Tucanae - Canvas - 12x12
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00CA1216
Globular Cluster 47 Tucanae - Canvas - 12x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00CA1616
Globular Cluster 47 Tucanae - Canvas - 16x16
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00CA1620
Globular Cluster 47 Tucanae - Canvas - 16x20
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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N0104V00CA1824
Globular Cluster 47 Tucanae - Canvas - 18x24
The heart of the giant Globular Cluster 47 Tucanae reveals the glow of 200,000 stars. Globular star clusters can be home to hundreds of thousands of stars, in constant motion, orbiting around the center of the cluster. In this cluster, Hubble shows a parade of young white dwarfs starting a 40-million-year migration away from the core. Observations show that in globular clusters the heavyweight stars reside in the crowded core, and lightweight stars live on the outskirts. Lower mass stars rob momentum from more massive stars causing the heavier stars sink to the core as their orbits slow, while the lighter stars pick up speed and move across the cluster to the edge. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: 47 Tucanae, NGC 104 Release Date: May 13, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy)
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REW03V00MP1218
Farmers Wanted - NASA Mars Explorers Wanted - Matte Paper - 12x18
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Matte Paper - 24x36
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Matte Framed - 12x18
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Matte Framed - 24x36
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Photo Paper - 12x18
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Photo Paper - 24x36
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Photo Framed - 12x18
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Photo Framed - 24x36
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Farmers Wanted - NASA Mars Explorers Wanted - Canvas - 24x36
We'll need farmers to grow food for our survival on Mars. Have you got a green thumb? Then you can be sure there is a place in space for you! We already know that tomatoes, lettuce, peas, and radishes can grow in space, just like you would find in your summer garden. But new and innovative ways of growing fresh food will be needed to keep brave explorers alive. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Matte Paper - 12x18
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Matte Paper - 24x36
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Matte Framed - 12x18
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Matte Framed - 24x36
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Photo Paper - 24x36
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Photo Framed - 12x18
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Photo Framed - 24x36
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Explorers Wanted - NASA Mars Explorers Wanted - Canvas - 24x36
Will you be a daring explorer on the Journey to Mars? Hike through the largest canyon in our solar system, the Valles Marineris on Mars, where you can witness blue sunsets in the twilight, and see the two moons of Mars (Phobos and Deimos) in the night sky. Someone is needed to help blaze the trail for all who will come after. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More NASA originally commissioned this poster as one of a set for an exhibit at the Kennedy Space Center Visitor's Complex in 2009.Image Credits: NASA/KSC
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Europa - NASA Visions of the Future - Matte Paper - 12x18
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Matte Paper - 24x36
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Matte Framed - 12x18
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Matte Framed - 24x36
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Photo Paper - 12x18
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Photo Paper - 24x36
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Photo Framed - 12x18
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Photo Framed - 24x36
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Europa - NASA Visions of the Future - Canvas - 24x36
What will NASA's Europa mission find when it heads toward Jupiter's intriguing moon in the 2020s? Europa's astonishing geology and the potential to host the conditions for simple life make this moon a fascinating destination for future exploration around Jupiter. Beneath the icy surface, it is believed the moon may conceal a global ocean of salty liquid water that is twice the volume of the oceans of Earth. Jupiter's gravity tugging and flexing the shape of the moon generates enough heat to keep the ocean from freezing. On Earth, when we find water, we find life. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 12x18
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 24x36
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 12x18
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 24x36
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 12x18
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 24x36
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 12x18
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 24x36
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Enceladus - NASA Visions of the Future - Canvas - 24x36
This tiny moon of Saturn is one of the leading locations in the search for possible life beyond Earth. The discovery of icy jets on Enceladus and their role in creating Saturn's E-ring is one of the top findings made by the Cassini probe mission to Saturn. Additional discoveries revealed strong evidence of a global ocean and the first signs of potential hydrothermal activity beyond Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Matte Paper - 12x18
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Matte Paper - 24x36
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Matte Framed - 12x18
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Matte Framed - 24x36
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Photo Paper - 12x18
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Photo Paper - 24x36
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Photo Framed - 12x18
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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RVF03V00PF2436
Earth - NASA Visions of the Future - Photo Framed - 24x36
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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Earth - NASA Visions of the Future - Canvas - 24x36
When Earth is the place that has all the right conditions for life, there is truly no place like home, yet. Of all the amazing beauty being revealed across our galaxy and throughout the universe, Earth is the only place we know of with life. When we tire of gazing skyward and travelling among the stars, there are plenty of miracles right here on Earth to enjoy. To make sure it stays that way, Earth science missions monitor our home planet and how it is changing so it can continue to provide a safe haven as we reach deeper into the cosmos. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series.Image Credits: Courtesy NASA/JPL-Caltech
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N6611V00MP0810
Eagle Nebula - M16 - Matte Paper - 8x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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Eagle Nebula - M16 - Matte Paper - 10x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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Eagle Nebula - M16 - Matte Paper - 12x12
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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Eagle Nebula - M16 - Matte Paper - 12x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MP1218
Eagle Nebula - M16 - Matte Paper - 12x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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Eagle Nebula - M16 - Matte Paper - 14x14
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MP1616
Eagle Nebula - M16 - Matte Paper - 16x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MP1620
Eagle Nebula - M16 - Matte Paper - 16x20
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MP1818
Eagle Nebula - M16 - Matte Paper - 18x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MP1824
Eagle Nebula - M16 - Matte Paper - 18x24
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MP2436
Eagle Nebula - M16 - Matte Paper - 24x36
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF0810
Eagle Nebula - M16 - Matte Framed - 8x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1010
Eagle Nebula - M16 - Matte Framed - 10x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1212
Eagle Nebula - M16 - Matte Framed - 12x12
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1216
Eagle Nebula - M16 - Matte Framed - 12x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1218
Eagle Nebula - M16 - Matte Framed - 12x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1414
Eagle Nebula - M16 - Matte Framed - 14x14
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1616
Eagle Nebula - M16 - Matte Framed - 16x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1620
Eagle Nebula - M16 - Matte Framed - 16x20
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1818
Eagle Nebula - M16 - Matte Framed - 18x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF1824
Eagle Nebula - M16 - Matte Framed - 18x24
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00MF2436
Eagle Nebula - M16 - Matte Framed - 24x36
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP0810
Eagle Nebula - M16 - Photo Paper - 8x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1010
Eagle Nebula - M16 - Photo Paper - 10x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1212
Eagle Nebula - M16 - Photo Paper - 12x12
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1216
Eagle Nebula - M16 - Photo Paper - 12x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1218
Eagle Nebula - M16 - Photo Paper - 12x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1414
Eagle Nebula - M16 - Photo Paper - 14x14
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1616
Eagle Nebula - M16 - Photo Paper - 16x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1620
Eagle Nebula - M16 - Photo Paper - 16x20
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1818
Eagle Nebula - M16 - Photo Paper - 18x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP1824
Eagle Nebula - M16 - Photo Paper - 18x24
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PP2436
Eagle Nebula - M16 - Photo Paper - 24x36
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF0810
Eagle Nebula - M16 - Photo Framed - 8x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1010
Eagle Nebula - M16 - Photo Framed - 10x10
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1212
Eagle Nebula - M16 - Photo Framed - 12x12
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1216
Eagle Nebula - M16 - Photo Framed - 12x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1218
Eagle Nebula - M16 - Photo Framed - 12x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1414
Eagle Nebula - M16 - Photo Framed - 14x14
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1616
Eagle Nebula - M16 - Photo Framed - 16x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1620
Eagle Nebula - M16 - Photo Framed - 16x20
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1818
Eagle Nebula - M16 - Photo Framed - 18x18
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF1824
Eagle Nebula - M16 - Photo Framed - 18x24
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00PF2436
Eagle Nebula - M16 - Photo Framed - 24x36
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00CA1212
Eagle Nebula - M16 - Canvas - 12x12
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00CA1216
Eagle Nebula - M16 - Canvas - 12x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00CA1616
Eagle Nebula - M16 - Canvas - 16x16
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00CA1620
Eagle Nebula - M16 - Canvas - 16x20
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00CA1824
Eagle Nebula - M16 - Canvas - 18x24
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N6611V00CA2436
Eagle Nebula - M16 - Canvas - 24x36
Hubble captures an improved view of the iconic "Pillars of Creation" with a sharper and wider view of pillars in the Eagle Nebula. In 1995, Hubble offered a breathtaking view of M16, the Eagle Nebula, which revealed details never seen before of three giant columns of cold gas. In celebration of the 25th anniversary of the original launch of the Hubble Space Telescope, the lens was once again aimed at M16 to revisit the famous spot with keener vision. The towering pillars seen are about 5 light-years tall and bathed in the blistering ultraviolet light of a group of young, massive stars located off the top of the image. Stars are being born deep inside the pillars, which are made of cold hydrogen gas laced with dust. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M16, Eagle Nebula, NGC 6611 Release Date: Apr 3, 2015 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N3034V00MP0810
Cigar Galaxy - M82 - Matte Paper - 8x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1010
Cigar Galaxy - M82 - Matte Paper - 10x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1212
Cigar Galaxy - M82 - Matte Paper - 12x12
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1216
Cigar Galaxy - M82 - Matte Paper - 12x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1218
Cigar Galaxy - M82 - Matte Paper - 12x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1414
Cigar Galaxy - M82 - Matte Paper - 14x14
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1616
Cigar Galaxy - M82 - Matte Paper - 16x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1620
Cigar Galaxy - M82 - Matte Paper - 16x20
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1818
Cigar Galaxy - M82 - Matte Paper - 18x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00MP1824
Cigar Galaxy - M82 - Matte Paper - 18x24
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
28.00
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N3034V00MP2436
Cigar Galaxy - M82 - Matte Paper - 24x36
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
36.00
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N3034V00MF0810
Cigar Galaxy - M82 - Matte Framed - 8x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
36.00
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N3034V00MF1010
Cigar Galaxy - M82 - Matte Framed - 10x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
42.00
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N3034V00MF1212
Cigar Galaxy - M82 - Matte Framed - 12x12
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
48.00
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N3034V00MF1216
Cigar Galaxy - M82 - Matte Framed - 12x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
54.00
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N3034V00MF1218
Cigar Galaxy - M82 - Matte Framed - 12x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
60.00
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N3034V00MF1414
Cigar Galaxy - M82 - Matte Framed - 14x14
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
60.00
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N3034V00MF1616
Cigar Galaxy - M82 - Matte Framed - 16x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
66.00
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N3034V00MF1620
Cigar Galaxy - M82 - Matte Framed - 16x20
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
72.00
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N3034V00MF1818
Cigar Galaxy - M82 - Matte Framed - 18x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
72.00
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N3034V00MF1824
Cigar Galaxy - M82 - Matte Framed - 18x24
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
84.00
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N3034V00MF2436
Cigar Galaxy - M82 - Matte Framed - 24x36
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
120.00
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N3034V00PP0810
Cigar Galaxy - M82 - Photo Paper - 8x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
16.00
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N3034V00PP1010
Cigar Galaxy - M82 - Photo Paper - 10x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
18.00
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N3034V00PP1212
Cigar Galaxy - M82 - Photo Paper - 12x12
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
20.00
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N3034V00PP1216
Cigar Galaxy - M82 - Photo Paper - 12x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
22.00
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N3034V00PP1218
Cigar Galaxy - M82 - Photo Paper - 12x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
24.00
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N3034V00PP1414
Cigar Galaxy - M82 - Photo Paper - 14x14
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
24.00
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N3034V00PP1616
Cigar Galaxy - M82 - Photo Paper - 16x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
26.00
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N3034V00PP1620
Cigar Galaxy - M82 - Photo Paper - 16x20
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
28.00
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N3034V00PP1818
Cigar Galaxy - M82 - Photo Paper - 18x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
28.00
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N3034V00PP1824
Cigar Galaxy - M82 - Photo Paper - 18x24
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
34.00
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N3034V00PP2436
Cigar Galaxy - M82 - Photo Paper - 24x36
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
40.00
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N3034V00PF0810
Cigar Galaxy - M82 - Photo Framed - 8x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00PF1010
Cigar Galaxy - M82 - Photo Framed - 10x10
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00PF1212
Cigar Galaxy - M82 - Photo Framed - 12x12
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
58.00
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N3034V00PF1216
Cigar Galaxy - M82 - Photo Framed - 12x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00PF1218
Cigar Galaxy - M82 - Photo Framed - 12x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00PF1414
Cigar Galaxy - M82 - Photo Framed - 14x14
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00PF1616
Cigar Galaxy - M82 - Photo Framed - 16x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
76.00
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N3034V00PF1620
Cigar Galaxy - M82 - Photo Framed - 16x20
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
82.00
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N3034V00PF1818
Cigar Galaxy - M82 - Photo Framed - 18x18
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
82.00
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N3034V00PF1824
Cigar Galaxy - M82 - Photo Framed - 18x24
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00PF2436
Cigar Galaxy - M82 - Photo Framed - 24x36
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
126.00
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N3034V00CA1212
Cigar Galaxy - M82 - Canvas - 12x12
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
54.00
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N3034V00CA1216
Cigar Galaxy - M82 - Canvas - 12x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
56.00
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N3034V00CA1616
Cigar Galaxy - M82 - Canvas - 16x16
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00CA1620
Cigar Galaxy - M82 - Canvas - 16x20
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00CA1824
Cigar Galaxy - M82 - Canvas - 18x24
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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N3034V00CA2436
Cigar Galaxy - M82 - Canvas - 24x36
Energetic plumes of hydrogen glow as they blast from the central nucleus of the Cigar galaxy. Stars are being born in the center of this galaxy 10 times faster than in our own Milky Way. The image of this starburst galaxy located in Ursa Major is the sharpest wide-angle view ever obtained of M82. This galaxy is remarkable because of its bright blue disk, webs of shredded clouds, and the fiery plumes of glowing hydrogen that blast out of its central regions. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: M82, NGC 3034, Cigar Galaxy Release Date: Apr 24, 2006 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
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RVF05V00MP1218
Ceres - NASA Visions of the Future - Matte Paper - 12x18
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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RVF05V00MP2436
Ceres - NASA Visions of the Future - Matte Paper - 24x36
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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RVF05V00MF1218
Ceres - NASA Visions of the Future - Matte Framed - 12x18
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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RVF05V00MF2436
Ceres - NASA Visions of the Future - Matte Framed - 24x36
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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RVF05V00PP1218
Ceres - NASA Visions of the Future - Photo Paper - 12x18
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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RVF05V00PP2436
Ceres - NASA Visions of the Future - Photo Paper - 24x36
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
40.00
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RVF05V00PF1218
Ceres - NASA Visions of the Future - Photo Framed - 12x18
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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RVF05V00PF2436
Ceres - NASA Visions of the Future - Photo Framed - 24x36
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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Ceres - NASA Visions of the Future - Canvas - 24x36
Ceres sits within the asteroid belt and was the first dwarf planet in our solar system explored by spacecraft. Ceres is the closest dwarf planet to our Sun and the largest object in the main asteroid belt between Mars and Jupiter. It has an equatorial diameter of only about 965 kilometers. It has been observed and studied with telescopes for more than two centuries. In March 2015, NASA's Dawn probe arrived in orbit around Ceres and it became the first dwarf planet to be explored by a spacecraft. The ongoing detailed observations by the probe are revealing interesting insights into this mysterious world of ice and rock. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More A creative team of visual strategists at JPL, known as "The Studio," created this image as part of the "Visions of the Future." poster series. Image Credits: Courtesy NASA/JPL-Caltech
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N3372V02MP0810
Carina Nebula Pillar - Matte Paper - 8x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02MP1010
Carina Nebula Pillar - Matte Paper - 10x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02MP1212
Carina Nebula Pillar - Matte Paper - 12x12
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02MP1216
Carina Nebula Pillar - Matte Paper - 12x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02MP1218
Carina Nebula Pillar - Matte Paper - 12x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02MP1414
Carina Nebula Pillar - Matte Paper - 14x14
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02MP1616
Carina Nebula Pillar - Matte Paper - 16x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
22.00
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N3372V02MP1620
Carina Nebula Pillar - Matte Paper - 16x20
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
24.00
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N3372V02MP1818
Carina Nebula Pillar - Matte Paper - 18x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
24.00
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N3372V02MP1824
Carina Nebula Pillar - Matte Paper - 18x24
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02MP2436
Carina Nebula Pillar - Matte Paper - 24x36
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
36.00
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N3372V02MF0810
Carina Nebula Pillar - Matte Framed - 8x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
36.00
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N3372V02MF1010
Carina Nebula Pillar - Matte Framed - 10x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
42.00
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N3372V02MF1212
Carina Nebula Pillar - Matte Framed - 12x12
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
48.00
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N3372V02MF1216
Carina Nebula Pillar - Matte Framed - 12x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
54.00
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N3372V02MF1218
Carina Nebula Pillar - Matte Framed - 12x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
60.00
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N3372V02MF1414
Carina Nebula Pillar - Matte Framed - 14x14
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
60.00
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N3372V02MF1616
Carina Nebula Pillar - Matte Framed - 16x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
66.00
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N3372V02MF1620
Carina Nebula Pillar - Matte Framed - 16x20
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
72.00
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N3372V02MF1818
Carina Nebula Pillar - Matte Framed - 18x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
72.00
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N3372V02MF1824
Carina Nebula Pillar - Matte Framed - 18x24
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
84.00
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N3372V02MF2436
Carina Nebula Pillar - Matte Framed - 24x36
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
120.00
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N3372V02PP0810
Carina Nebula Pillar - Photo Paper - 8x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP1010
Carina Nebula Pillar - Photo Paper - 10x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP1212
Carina Nebula Pillar - Photo Paper - 12x12
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP1216
Carina Nebula Pillar - Photo Paper - 12x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP1218
Carina Nebula Pillar - Photo Paper - 12x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP1414
Carina Nebula Pillar - Photo Paper - 14x14
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
24.00
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N3372V02PP1616
Carina Nebula Pillar - Photo Paper - 16x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP1620
Carina Nebula Pillar - Photo Paper - 16x20
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP1818
Carina Nebula Pillar - Photo Paper - 18x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
28.00
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N3372V02PP1824
Carina Nebula Pillar - Photo Paper - 18x24
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
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N3372V02PP2436
Carina Nebula Pillar - Photo Paper - 24x36
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
40.00
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N3372V02PF0810
Carina Nebula Pillar - Photo Framed - 8x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
46.00
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N3372V02PF1010
Carina Nebula Pillar - Photo Framed - 10x10
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
52.00
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N3372V02PF1212
Carina Nebula Pillar - Photo Framed - 12x12
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
58.00
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N3372V02PF1216
Carina Nebula Pillar - Photo Framed - 12x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
64.00
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N3372V02PF1218
Carina Nebula Pillar - Photo Framed - 12x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
70.00
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N3372V02PF1414
Carina Nebula Pillar - Photo Framed - 14x14
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
70.00
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N3372V02PF1616
Carina Nebula Pillar - Photo Framed - 16x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
76.00
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N3372V02PF1620
Carina Nebula Pillar - Photo Framed - 16x20
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
82.00
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N3372V02PF1818
Carina Nebula Pillar - Photo Framed - 18x18
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
82.00
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N3372V02PF1824
Carina Nebula Pillar - Photo Framed - 18x24
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
100.00
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N3372V02PF2436
Carina Nebula Pillar - Photo Framed - 24x36
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
126.00
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N3372V02CA1212
Carina Nebula Pillar - Canvas - 12x12
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
54.00
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N3372V02CA1216
Carina Nebula Pillar - Canvas - 12x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
56.00
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N3372V02CA1616
Carina Nebula Pillar - Canvas - 16x16
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
58.00
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N3372V02CA1620
Carina Nebula Pillar - Canvas - 16x20
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
60.00
https://posternauts.com/products/carina-nebula-pillar?variant=35118719944
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https://posternauts.com/cdn/shop/products/ps49-canvas-16x20_medium.png?v=1496949220,
N3372V02CA1824
Carina Nebula Pillar - Canvas - 18x24
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
70.00
https://posternauts.com/products/carina-nebula-pillar?variant=35118720072
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https://posternauts.com/cdn/shop/products/ps49-canvas-18x24_medium.png?v=1496949220,
N3372V02CA2436
Carina Nebula Pillar - Canvas - 24x36
A pillar of gas in the Carina Nebula is bathed in the light of hot, massive stars. There are many beauties to be found within the Carina Nebula, including the Carina Nebula Pillar. Radiation and fast winds from the stars sculpt the pillar of gas in this image and cause new star formation within it.There are over 14,000 stars within the region of this nebula and there is evidence that massive stars have self-destructed in supernova explosions that took place here. But these same destructive forces cause the formation of new, bright stars within pillars such as this one. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Jet in Carina Release Date: Sep 9, 2009 Image Credits: NASA, ESA, and the Hubble SM4 ERO Team
100.00
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N3372V00MP0810
Carina Nebula - NGC 3372 - Canvas - 8x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
12.00
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N3372V00MP1010
Carina Nebula - NGC 3372 - Canvas - 10x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
14.00
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N3372V00MP1212
Carina Nebula - NGC 3372 - Canvas - 12x12
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
16.00
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N3372V00MP1216
Carina Nebula - NGC 3372 - Canvas - 12x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
18.00
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N3372V00MP1218
Carina Nebula - NGC 3372 - Canvas - 12x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
20.00
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N3372V00MP1414
Carina Nebula - NGC 3372 - Canvas - 14x14
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
20.00
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N3372V00MP1616
Carina Nebula - NGC 3372 - Canvas - 16x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
22.00
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N3372V00MP1620
Carina Nebula - NGC 3372 - Canvas - 16x20
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
24.00
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N3372V00MP1818
Carina Nebula - NGC 3372 - Canvas - 18x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
24.00
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N3372V00MP1824
Carina Nebula - NGC 3372 - Canvas - 18x24
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
28.00
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N3372V00MP2436
Carina Nebula - NGC 3372 - Canvas - 24x36
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
36.00
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N3372V00MF0810
Carina Nebula - NGC 3372 - Canvas - 8x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
36.00
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N3372V00MF1010
Carina Nebula - NGC 3372 - Canvas - 10x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
42.00
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N3372V00MF1212
Carina Nebula - NGC 3372 - Canvas - 12x12
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
48.00
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N3372V00MF1216
Carina Nebula - NGC 3372 - Canvas - 12x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
54.00
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N3372V00MF1218
Carina Nebula - NGC 3372 - Canvas - 12x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
60.00
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N3372V00MF1414
Carina Nebula - NGC 3372 - Canvas - 14x14
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
60.00
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N3372V00MF1616
Carina Nebula - NGC 3372 - Canvas - 16x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
66.00
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N3372V00MF1620
Carina Nebula - NGC 3372 - Canvas - 16x20
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
72.00
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N3372V00MF1818
Carina Nebula - NGC 3372 - Canvas - 18x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
72.00
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N3372V00MF1824
Carina Nebula - NGC 3372 - Canvas - 18x24
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
84.00
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N3372V00MF2436
Carina Nebula - NGC 3372 - Canvas - 24x36
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
120.00
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N3372V00PP0810
Carina Nebula - NGC 3372 - Canvas - 8x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
16.00
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N3372V00PP1010
Carina Nebula - NGC 3372 - Canvas - 10x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
18.00
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N3372V00PP1212
Carina Nebula - NGC 3372 - Canvas - 12x12
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
20.00
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N3372V00PP1216
Carina Nebula - NGC 3372 - Canvas - 12x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
22.00
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N3372V00PP1218
Carina Nebula - NGC 3372 - Canvas - 12x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
24.00
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N3372V00PP1414
Carina Nebula - NGC 3372 - Canvas - 14x14
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
24.00
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N3372V00PP1616
Carina Nebula - NGC 3372 - Canvas - 16x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
26.00
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N3372V00PP1620
Carina Nebula - NGC 3372 - Canvas - 16x20
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
28.00
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N3372V00PP1818
Carina Nebula - NGC 3372 - Canvas - 18x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
28.00
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N3372V00PP1824
Carina Nebula - NGC 3372 - Canvas - 18x24
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
34.00
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N3372V00PP2436
Carina Nebula - NGC 3372 - Canvas - 24x36
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
40.00
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N3372V00PF0810
Carina Nebula - NGC 3372 - Canvas - 8x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
46.00
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N3372V00PF1010
Carina Nebula - NGC 3372 - Canvas - 10x10
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
52.00
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N3372V00PF1212
Carina Nebula - NGC 3372 - Canvas - 12x12
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
58.00
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N3372V00PF1216
Carina Nebula - NGC 3372 - Canvas - 12x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
64.00
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N3372V00PF1218
Carina Nebula - NGC 3372 - Canvas - 12x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
70.00
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N3372V00PF1414
Carina Nebula - NGC 3372 - Canvas - 14x14
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
70.00
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N3372V00PF1616
Carina Nebula - NGC 3372 - Canvas - 16x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
76.00
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N3372V00PF1620
Carina Nebula - NGC 3372 - Canvas - 16x20
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
82.00
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N3372V00PF1818
Carina Nebula - NGC 3372 - Canvas - 18x18
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
82.00
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N3372V00PF1824
Carina Nebula - NGC 3372 - Canvas - 18x24
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
100.00
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N3372V00PF2436
Carina Nebula - NGC 3372 - Canvas - 24x36
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
126.00
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N3372V00CA1212
Carina Nebula - NGC 3372 - Canvas - 12x12
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
54.00
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N3372V00CA1216
Carina Nebula - NGC 3372 - Canvas - 12x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
56.00
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N3372V00CA1616
Carina Nebula - NGC 3372 - Canvas - 16x16
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
58.00
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N3372V00CA1620
Carina Nebula - NGC 3372 - Canvas - 16x20
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
60.00
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N3372V00CA1824
Carina Nebula - NGC 3372 - Canvas - 18x24
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
70.00
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N3372V00CA2436
Carina Nebula - NGC 3372 - Canvas - 24x36
A region of star birth and death in the Carina Nebula is so impressive, it is also known as the Grand Nebula. This image, released for Hubble's 17th anniversary, displays a 50 light-year wide view of the central region inside the Carina Nebula, within the Carina-Sagittarius Arm of the constellation Carina. The nebula is estimated to be between 6,500 and 10,000 light-years from Earth and is somewhat lesser known because of its location in our southern sky. There are at least a dozen brilliant stars that are 50 to 100 times the mass of our Sun within this maelstrom of star birth and death. Red represents the presence of sulfur, green is hydrogen, and blue is oxygen emission. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Carina Nebula, NGC 3372 Release Date: Apr 24, 2007 Image Credits: Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA); Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF
100.00
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N7635V00MP0810
Bubble Nebula - NGC 7635 - Matte Paper - 8x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
12.00
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N7635V00MP1010
Bubble Nebula - NGC 7635 - Matte Paper - 10x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
14.00
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N7635V00MP1212
Bubble Nebula - NGC 7635 - Matte Paper - 12x12
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
16.00
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N7635V00MP1216
Bubble Nebula - NGC 7635 - Matte Paper - 12x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
18.00
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N7635V00MP1218
Bubble Nebula - NGC 7635 - Matte Paper - 12x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
20.00
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N7635V00MP1414
Bubble Nebula - NGC 7635 - Matte Paper - 14x14
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
20.00
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N7635V00MP1616
Bubble Nebula - NGC 7635 - Matte Paper - 16x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
22.00
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N7635V00MP1620
Bubble Nebula - NGC 7635 - Matte Paper - 16x20
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
24.00
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N7635V00MP1818
Bubble Nebula - NGC 7635 - Matte Paper - 18x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
24.00
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N7635V00MP1824
Bubble Nebula - NGC 7635 - Matte Paper - 18x24
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
28.00
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N7635V00MP2436
Bubble Nebula - NGC 7635 - Matte Paper - 24x36
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
36.00
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N7635V00MF0810
Bubble Nebula - NGC 7635 - Matte Framed - 8x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
36.00
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N7635V00MF1010
Bubble Nebula - NGC 7635 - Matte Framed - 10x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
42.00
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N7635V00MF1212
Bubble Nebula - NGC 7635 - Matte Framed - 12x12
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
48.00
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N7635V00MF1216
Bubble Nebula - NGC 7635 - Matte Framed - 12x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
54.00
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N7635V00MF1218
Bubble Nebula - NGC 7635 - Matte Framed - 12x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
60.00
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N7635V00MF1414
Bubble Nebula - NGC 7635 - Matte Framed - 14x14
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
60.00
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N7635V00MF1616
Bubble Nebula - NGC 7635 - Matte Framed - 16x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
66.00
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N7635V00MF1620
Bubble Nebula - NGC 7635 - Matte Framed - 16x20
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
72.00
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N7635V00MF1818
Bubble Nebula - NGC 7635 - Matte Framed - 18x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
72.00
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N7635V00MF1824
Bubble Nebula - NGC 7635 - Matte Framed - 18x24
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
84.00
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N7635V00MF2436
Bubble Nebula - NGC 7635 - Matte Framed - 24x36
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
120.00
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N7635V00PP0810
Bubble Nebula - NGC 7635 - Photo Paper - 8x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
16.00
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N7635V00PP1010
Bubble Nebula - NGC 7635 - Photo Paper - 10x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
18.00
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N7635V00PP1212
Bubble Nebula - NGC 7635 - Photo Paper - 12x12
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
20.00
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N7635V00PP1216
Bubble Nebula - NGC 7635 - Photo Paper - 12x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
22.00
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N7635V00PP1218
Bubble Nebula - NGC 7635 - Photo Paper - 12x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
24.00
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N7635V00PP1414
Bubble Nebula - NGC 7635 - Photo Paper - 14x14
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
24.00
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N7635V00PP1616
Bubble Nebula - NGC 7635 - Photo Paper - 16x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
26.00
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N7635V00PP1620
Bubble Nebula - NGC 7635 - Photo Paper - 16x20
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
28.00
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N7635V00PP1818
Bubble Nebula - NGC 7635 - Photo Paper - 18x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
28.00
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N7635V00PP1824
Bubble Nebula - NGC 7635 - Photo Paper - 18x24
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N7635V00PP2436
Bubble Nebula - NGC 7635 - Photo Paper - 24x36
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N7635V00PF0810
Bubble Nebula - NGC 7635 - Photo Framed - 8x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N7635V00PF1010
Bubble Nebula - NGC 7635 - Photo Framed - 10x10
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N7635V00PF1212
Bubble Nebula - NGC 7635 - Photo Framed - 12x12
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
58.00
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N7635V00PF1216
Bubble Nebula - NGC 7635 - Photo Framed - 12x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
64.00
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N7635V00PF1218
Bubble Nebula - NGC 7635 - Photo Framed - 12x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
70.00
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N7635V00PF1414
Bubble Nebula - NGC 7635 - Photo Framed - 14x14
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
70.00
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N7635V00PF1616
Bubble Nebula - NGC 7635 - Photo Framed - 16x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
76.00
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N7635V00PF1620
Bubble Nebula - NGC 7635 - Photo Framed - 16x20
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
82.00
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N7635V00PF1818
Bubble Nebula - NGC 7635 - Photo Framed - 18x18
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
82.00
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N7635V00PF1824
Bubble Nebula - NGC 7635 - Photo Framed - 18x24
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
100.00
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N7635V00PF2436
Bubble Nebula - NGC 7635 - Photo Framed - 24x36
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
126.00
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N7635V00CA1212
Bubble Nebula - NGC 7635 - Canvas - 12x12
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
54.00
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N7635V00CA1216
Bubble Nebula - NGC 7635 - Canvas - 12x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
56.00
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N7635V00CA1616
Bubble Nebula - NGC 7635 - Canvas - 16x16
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
58.00
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N7635V00CA1620
Bubble Nebula - NGC 7635 - Canvas - 16x20
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
60.00
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N7635V00CA1824
Bubble Nebula - NGC 7635 - Canvas - 18x24
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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N7635V00CA2436
Bubble Nebula - NGC 7635 - Canvas - 24x36
The Bubble Nebula is the result of hot gas which is escaping into space from a star 45 times more massive than our Sun. Hubble captured this balloon-like sphere of gas being blown into space by a super-hot, massive star. The bubble is 7 light-years across, which is one-and-a-half times greater than the distance from the Sun to our nearest stellar neighbor, Alpha Centauri. The Bubble Nebula lies in the constellation Cassiopeia, approximately 7,100 light-years from Earth. A portion of every Posternauts purchase supports young minds through the scholarship fund of the U.S. Space & Rocket Center® Foundation. Learn More Object Name: Bubble Nebula, NGC 7635 Release Date: Apr 20, 2016 Image Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
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