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Space observatory
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A space observatory is any instrument in outer space which is used for observation of distant planets, galaxies, and other outer space objects. This category is distinct from other observatories located in space that are pointed toward the earth for the purpose of reconnaissance and other types of information gathering.
rge number of observatories have been launched into orbit, and most of them have greatly enhanced our knowledge of the Cosmos.

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A space observatory is any instrument in outer space which is used for observation of distant planets, galaxies, and other outer space objects. This category is distinct from other observatories located in space that are pointed toward the earth for the purpose of reconnaissance and other types of information gathering.
Introduction
A large number of observatories have been launched into orbit, and most of them have greatly enhanced our knowledge of the Cosmos. Performing astronomy from the Earth's surface is limited by the filtering and distortion of electromagnetic radiation due to the Earth's atmosphere. This makes it desirable to place astronomical observation devices into space. As a telescope orbits the Earth outside the atmosphere it is subject neither to twinkling (distortion due to thermal turbulences of the air) nor to light pollution from artificial light sources on the Earth. Some terrestrial telescopes (such as the Very Large Telescope) can counter turbulences with the help of their novel adaptive optics.
But space-based astronomy is even more important for frequency ranges which are outside of the optic window and the radio window, the only two wavelength ranges of the electromagnetic spectrum that are not severely attenuated by the atmosphere. For example, X-ray astronomy is nearly impossible when done from the Earth, and has reached its current important stand within astronomy only due to orbiting satellites with X-ray telescopes such as the Chandra observatory or XMM-Newton observatory. Infrared and ultraviolet are also greatly blocked.
Space observatories can generally be divided into two classes: missions
which map the entire sky (surveys), and observatories which make observations of chosen parts of the sky.
Many space observatories have already completed their missions, while others are still operating. Satellites have been launched and operated by NASA, ESA, Japanese Space Agency and the Soviet space program later succeeded by Roskosmos of Russia.
NASA's Great Observatories Satellites belonging to NASA's "Great Observatories" program:
- The Gamma ray Observatory (GRO), since renamed to The Compton Gamma-Ray Observatory, had to be disposed of after several years of productive life. Its gyroscopes began to fail and when it was down to its last gyroscope, the choice was to risk losing control or destroying the observatory. NASA de-orbited the bus-sized satellite into the Pacific Ocean in 2000.
- X-Rays are also represented in the Great Observatories, with the Chandra X-ray Observatory (CXO), renamed (from AXAF - Advanced X-Ray Astrophysics Facility) in honor of the Indian astrophysicist Chandrasekhar. This has been used to great effect to study distant galaxies and is still operational.
Other active space observatories
- SOHO - solar observatory, operational since 1995, used for the study of the Sun's corona and magnetic environments. SOHO has revolutionised our knowledge of the Sun.
- WMAP (Wilkinson Microwave Anisotropy Probe) - probes Big Bang by analyzing cosmic background radiation. In operation since 2001.
MOST (Microvariability and Oscillations of STars telescope) the smallest space telescope in the world, the size of a small chest or very large suitcase. Launched in 2003; expected to operate five years.
Swift (Swift Gamma-Ray Burst Mission) - launched in 2004 to detect and study gamma ray bursts.
ASTRO-EII (Suzaku) - launched in February 2006, suffered a mechanical fault a month after launch. Designed for high-resolution wide-band spectroscopy, it is operating at reduced levels.
AKARI (ASTRO-F) - launched in February 2006, intened to deep-map the entire sky in mid infrared and far infrared wavelengths.
- COROT - observatory launched in December 2006. It is the first mission to search for rocky worlds around other stars.
Kepler - space photometer launched in March 2009 to detect Earth-like and smaller planets by the transit method.
Decommissioned space observatories
- Uhuru (SAS-1) - the first X-ray space observatory. Operated 1970-1973.
- SAS-2 - gamma-ray observatory, also known as Explorer 48. Operated 1972-1973.
ANS - X-ray and ultraviolet space observatory launched in 1974 and active until 1976; the first to detect X-ray bursts
- SAS-3 - X-ray space observatory, also known as Explorer 53. Operated 1975-1979.
HEAO 1 (High Energy Astronomy Observatory 1) - X-Ray space observatory, operational 1977-1979.
- IUE (International Ultraviolet Explorer) - multinational observatory launched in 1978. Though intended for a planned lifetime of only 3 years, not deactivated until 1996.
HEAO 2 (Einstein Observatory) - X-Ray space observatory, operational 1978-1982.
HEAO 3 (High Energy Astronomy Observatory 3) - X-Ray space observatory, operational 1979-?.
- IRAS (Infrared Astronomical Satellite) - launched in 1983, it carried out the first all-sky infrared survey, as well as discovering disks of dust and gas around many nearby stars, including Fomalhaut, Vega and Beta Pictoris. Ceased functioning after ten months.
- EXOSAT - X-ray observatory, active 1983-1986.
- Astron - ultraviolet telescope, operated from 1983 to 1989.
- Granat - x- and gamma-ray telescope complex, operated from 1989 to 1998.
- - Hipparcos - satellite for measuring stellar parallax, active 1989-1993. Despite significant operational problems, it revised the Cepheid variable star distance scale to great accuracy and has been invaluable for all branches of observational astronomy by furnishing scientists with extremely accurate "standard candles" for measuring distances.
- ISO (Infrared Space Observatory) - 1995-1998 follow-on mission to IRAS; like it, carried out observations at infra-red wavelengths.
FUSE - operated from 1999 to 2007, making observations in the far UV portion of the spectrum.
- SCISAT-1 - analyzed Earth's upper atmosphere with an optical Fourier transform infrared spectrometer. Active 2003-2005.
Future space observatories
ESA candidate observatories in the 2015-2025 timeframe
- DUNE, intended to survey the entire sky in the optical and infra-red wavelength at a uniform 0.1 arcsecond resolution to allow accurate measurements of gravitational lensing to determine the distribution of dark matter within galaxy clusters
- SPACE, intended to take near-IR spectra of half a billion galaxies
- PLATO, a sequel to Kepler and Corot comprising many small telescopes with large CCD detectors on a single spacecraft, intended to provide precision photometry over a thousand square degrees of sky. This is similar to the cancelled Eddington mission.
- SPICA, in collaboration with the Japanese space agency; this is a large infra-red telescope with cryogenic optics designed to work with unprecedented sensitivity in the 5-200um wavelength range.
- XEUS, a X-ray space observatory with the mirror (using micro-pore optics) and detectors on separate spacecraft flying in formation.
See also
External links
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