NASA Technical Reports Server (NTRS) : Overview pdf

NASA Technical Reports Server (NTRS) : Overview

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The Chandra X-Ray Observatory (originally called the Advanced X-Ray Astrophysics Facility – AXAF) is the X-Ray component of NASA’s “Great Observatory” Program. Chandra is a NASA facility that provides scientific data to the international astronomical community in response to scientific proposals for its use. The Observatory is the product of the efforts of many organizations in the United States and Europe. The Great Observatories also include the Hubble Space Telescope for space-based observations of astronomical objects primarily in the visible portion of the electromagnetic spectrum, the now defunct Compton Gamma- Ray Observatory that was designed to observe gamma-ray emission from astronomical objects, and the soon-to-be-launched Space Infrared Telescope Facility (SIRTF). The Chandra X-Ray Observatory (hereafter CXO) is sensitive to X-rays in the energy range from below 0.1 to above 10.0 keV corresponding to wavelengths from 12 to 0.12 nanometers. The relationship among the various parts of the electromagnetic spectrum, sorted by characteristic temperature and the corresponding wavelength, is illustrated.

The German physicist Wilhelm Roentgen discovered what he thought was a new form of radiation in 1895. He called it X-radiation to summarize its properties. The radiation had the ability to pass through many materials that easily absorb visible light and to free electrons from atoms. We now know that X-rays are nothing more than light (electromagnetic radiation) but at high energies. Light has been given many names: radio waves, microwaves, infrared, visible, ultraviolet, X-ray and gamma radiation are all different forms. Radio waves are composed of low energy particles of light (photons). Optical photons – the only photons perceived by the human eye – are a million times more energetic than the typical radio photon, whereas the energies of X-ray photons range from hundreds to thousands of times higher than that of optical photons. Very low temperature systems (hundreds of degrees below zero Celsius) produce low energy radio and microwave photons, whereas cool bodies like our own (about 30 degrees Celsius) produce infrared radiation.

Very high temperatures (millions of degrees Celsius) are one way of producing X-rays

• Creator/s: NASA Technical Reports Server (NTRS
• Date: 1/1/2002
• Year: 2002
• Book Topics/Themes: NASA Technical Reports Server (NTRS), SPACE INFRARED TELESCOPE FACILITY, X RAY ASTROPHYSICS FACILITY, ASTROPHYSICS, GAMMA RAY OBSERVATORY, NASA SPACE PROGRAMS, X RAY ASTRONOMY, ELECTROMAGNETIC SPECTRA, PHOTONS, PARTICLE ENERGY, LOW TEMPERATURE, INFRARED RADIATION, QUASARS, GAMMA RAY BURSTS, Weisskopf, M. C

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