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A little bit of History

X-ray astronomy began with the detection of x-rays from the Sun in 1949, and from celestial sources outside the solar system in 1962. Unlike optical EM radiation, which we can see, or infrared radiation, which we can feel as heat, X-rays cannot be detected directly by a person. Since their discovery, scientists have refined ways of observing X-rays from outer space. Since X-rays do not penetrate the Earth's atmosphere, instruments to detect them have to be flown on satellites above the atmosphere. X-ray satellites can have instruments that record image data, spectral data, timing data or any combination of the three. Many X-ray satellites observe the same sources, or even the entire sky, over a long time, taking "timing data." Examples of satellites that took timing data, with links to pages on those satellites and their instruments, are:

artist's conception of Vela 5B
Vela 5B (1960s)
artist's concption of OSO 8
OSO-8 (1970s)
artist's conception of EXOSAT
artist's conception on RXTE
RXTE (1990s)

If words seem to be missing from the articles, please read this.

Imagine the Universe! is a service of the High Energy Astrophysics Science Archive Research Center (HEASARC), Dr. Alan Smale (Director), within the Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center.

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All material on this site has been created and updated between 1997-2014.
This page last updated: Wednesday, 06-Sep-2006 14:45:51 EDT