Ultraviolet Astronomy

Ultraviolet astronomy is generally used to refer to observations of electromagnetic radiation at ultraviolet wavelengths between approximately 10 and 320 nanometres; shorter wavelengths—higher energy photons—are studied by X-ray astronomy and gamma ray astronomy. Light at these wavelengths is absorbed by the Earth's atmosphere, so observations at these wavelengths must be performed from the upper atmosphere or from space.

Ultraviolet line spectrum measurements are used to discern the chemical composition, densities, and temperatures of the interstellar medium, and the temperature and composition of hot young stars. UV observations can also provide essential information about the evolution of galaxies.

The ultraviolet Universe looks quite different from the familiar stars and galaxies seen in visible light. Most stars are actually relatively cool objects emitting much of their electromagnetic radiation in the visible part of the spectrum. Ultraviolet radiation is the signature of hotter objects, typically in the early and late stages of their evolution. If we could see the sky in ultraviolet light, most stars would fade in prominence. We would see some very young massive stars and some very old stars and galaxies, growing hotter and producing higher-energy radiation near their birth or death. Clouds of gas and dust would block our vision in many directions along the Milky Way.

The Hubble Space Telescope and FUSE have been the most recent major space telescopes to view the near and far UV spectrum of the sky, though other UV instruments have flown on sounding rockets and the Space Shuttle.

Read more about Ultraviolet Astronomy:  Ultraviolet Space Telescopes

Other articles related to "ultraviolet astronomy, ultraviolet":

Observational Astronomy - Ultraviolet Astronomy
... Ultraviolet astronomy is generally used to refer to observations at ultraviolet wavelengths between approximately 100 and 3200 Å (10 to 320 nm) ... Ultraviolet astronomy is best suited to the study of thermal radiation and spectral emission lines from hot blue stars (OB stars) that are very bright in this wave band ... This includes the blue stars in other galaxies, which have been the targets of several ultraviolet surveys ...
Ultraviolet Astronomy - Ultraviolet Space Telescopes
... Netherlands Satellite (150-330 nm, 1974–76) + ESA - Extreme ultraviolet Imaging Telescope (on SOHO imaging sun at 17.1, 19.5, 28.4, and 30.4 nm) EUVE (7-76 nm, 1992-2001) - FUSE (90.5-119.5 nm, 1999-2007) - GALEX (13 ... Mission (170–650 nm spectra, 2004-- ) - Hopkins Ultraviolet Telescope (flew in 1990 and 1995) - ROSAT XUV (17-210eV) (30-6 nm, 1990-1999) See also List_of_space_telescopes#Ultraviolet ...
1967 In Spaceflight - Launches
... RAE/WRE (none) N/A N/A Solar X-ray and Ultraviolet observation N/A Successful April 0032 ... GMT Skylark 3 LA-2-SL, Woomera RAE/WRE (none) N/A N/A Ionosphere research N/A Successful April 8 0900 ...

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