Space observatory

From Academic Kids

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



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 neither subject 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. 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 by NASA, ESA and the Japanese Space Agency.

NASA's Great Observatories

Satellites belonging to NASA's "Great Observatories" program:

  • The Space Telescope (ST), now known as Hubble Space Telescope (HST) is the optical Great Observatory. It was launched to great acclaim and soon after discovered to be flawed. Its main mirror contained imperfections in its grinding that resulted from a certain production limitation being accounted for twice. It has now been fitted with the equivalent of spectacles to compensate for this.

Other notable space observatories

  • IRAS, which 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. This ceased functioning in 1982 and has since re-entered the atmosphere.
  • 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, the first (1970) X-Ray space observatory.
  • HEAO (High Energy Astronomy Observatories) 1 and 2, subsequent (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 last five years.

Future space observatories

See also

es:Observatorio espacial it:Telescopio spaziale nl:Ruimtetelescoop fi:Avaruustutkimusasema


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