Space observatory

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Space observatories
Space observatories and their wavelength working ranges
Website
http://nssdc.gsfc.nasa.gov/astro/astrolist.html
Space Observatories and their wavelength working range. Inspired by http://www.spitzer.caltech.edu/Media/mediaimages/background.shtml
Space Observatories and their wavelength working range. Inspired by http://www.spitzer.caltech.edu/Media/mediaimages/background.shtml
Spitzer, Hubble and XMM with their most important parts depicted
Spitzer, Hubble and XMM with their most important parts depicted

A space observatory is any instrument in outer space which is used for observation of distant planets, galaxies, and other outer space objects.

Contents

[edit] 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 astrononomical 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.

[edit] 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.

[edit] Other notable space observatories

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  • IRAS performed an all-sky survey in infrared, as well as discovering disks of dust and gas around many nearby stars, such as Fomalhaut, Vega and Beta Pictoris. IRAS ceased functioning in 1983 and continues to orbit at a height near 800 kilometres.
  • Granat, a Soviet x-ray and gamma-ray telescope complex, operated from 1989 to 1998.
  • COROT space telescope, a French Space Agency/ESA observatory that was launched in December 2006. It is the first mission to search for rocky worlds around other stars.
  • IUE (International Ultraviolet Explorer), an ESA/NASA/UK observatory that was launched in 1978 with a planned lifetime of 3 years. It was eventually switched off in 1996.
  • SOHO is a solar observatory that is currently operational and used for the study of the Sun's corona and magnetic environments. SOHO has revolutionised our knowledge of the Sun.
  • SCISAT-1 is a Canadian satellite which observes Earth's upper atmosphere with an optical Fourier transform infrared spectrometer.
  • Uhuru was the first (1970) X-Ray space observatory.
  • ANS was a Dutch X-ray and ultraviolet space observatory launched in 1974 and was the first to detect X-ray bursts.
  • HEAO (High Energy Astronomy Observatories) 1 and 2, subsequent (1977, 1978) X-Ray space observatories.
  • Hipparcos was a satellite for measuring stellar parallax. 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.
  • MOST was launched in 2003 for the Canadian Space Agency and it is the smallest space telescope in the world, being the size of a small chest or a very large suitcase. It is expected to operate five years.
  • FUSE operated from 1999 to 2007, making observations in the far UV.

[edit] Future space observatories

[edit] See also

[edit] External Links

Virtual Telescope retrieved May 13, 2008