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The world's first infrared astronomical satellite
Collaboration between the United States, the Netherlands and the United Kingdom
Telescope Aperture |
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60 cm |
Satellite Gross Weight |
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1073 kg |
Mission Lifespan |
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10 months |
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Discovery of many new celestial bodies, such as dust clouds, which are believed to be evidence of the formation of planets surrounding bright galaxies and stars, as seem by far-infrared light. |
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Japan's first infrared space telescope
The telescope was carried on the multipurpose observation satellite SFU, with other instruments.
Telescope Aperture |
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15 cm |
Telescope Weight |
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200 kg (the gross weight of the SFU satellite was 3850 kg) |
Mission Lifespan |
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approx. 1 month |
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By precisely measuring the background radiation in the universe, which appears to be pitch-black, IRTS observed extremely distant galaxies, and detected what scientists believe is the light of the first star formed in the universe. |
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IRTS detected organic compounds existing broadly in the universe. These molecules, consisting only of carbon and hydrogen, turned out to be PAHs (polycyclic aromatic hydrocarbons), a type of benzene related to biological processes. |
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Infrared space observatory, for detailed study of individual celestial bodies and specific regions of the universe
Project by the European Space Agency (ESA)
Telescope Aperture |
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60 cm |
Satellite Gross Weight |
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2400 kg |
Mission Lifespan |
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2.5 years |
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Crystals similar to those found on Earth were found in cosmic dust. This discovery has lead to a new, deeper study looking at the evolution of minerals (solid materials) in space. |
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Spitzer was launched as part of NASA's Great Observatories program, which includes the Hubble Space Telescope. The mission continues to this day.
Telescope Aperture |
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85 cm |
Satellite Gross Weight |
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923 kg |
Mission Lifespan |
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2.5 to 5 years (scheduled) |
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These are images of a galaxy forming several billion light years away. This kind of observation allows detailed study of star formation, galaxy evolution and planetary formation. |
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Spitzer succeeded in observing extrasolar planets directly. |
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