Compton Gamma Ray Observatory
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Home > Art, Film & Photography > Compton Gamma Ray Observatory: Energetic Gamma Ray Experiment Telescope, Grb 990123, 3c 279
Compton Gamma Ray Observatory: Energetic Gamma Ray Experiment Telescope, Grb 990123, 3c 279

Compton Gamma Ray Observatory: Energetic Gamma Ray Experiment Telescope, Grb 990123, 3c 279


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About the Book

Chapters: Energetic Gamma Ray Experiment Telescope, Grb 990123, 3c 279. Source: Wikipedia. Pages: 24. Not illustrated. Free updates online. Purchase includes a free trial membership in the publisher's book club where you can select from more than a million books without charge. Excerpt: The Compton Gamma Ray Observatory (CGRO) was the second of the NASA "Great Observatories" to be launched to space, following the Hubble Space Telescope. CGRO was named after Dr. Arthur Holly Compton (Washington University in St. Louis), Nobel prize winner, for work involved with gamma ray physics. CGRO was built by TRW (now Northrop Grumman Aerospace Systems) in Redondo Beach, CA. Following 14 years of effort, the observatory was launched on the Space Shuttle Atlantis, mission STS-37, on 5 April 1991 and operated until its deorbit on 4 June 2000. It was deployed in low earth orbit at 450 km (280 miles) to avoid the Van Allen radiation belt. It was the heaviest astrophysical payload ever flown at that time at 17,000 kilograms (37,000 lb). The CGRO is part of NASA's Great Observatories series, with the Hubble Space Telescope, the Chandra X-ray Observatory, and the Spitzer Space Telescope. CGRO carried a complement of four instruments that covered an unprecedented six decades of the electromagnetic spectrum, from 20 keV to 30 GeV. In order of increasing spectral energy coverage: The Compton Gamma Ray Observatory during deployment from STS-37 The Moon as seen by the Compton Gamma Ray Observatory, in gamma rays of greater than 20 MeV. These are produced by cosmic ray bombardment of its surface. The Sun, which has no similar surface of high atomic number to act as target for cosmic rays, cannot be seen at all at these energies, which are too high to emerge from primary nuclear reactions, such as solar nuclear fusion. Gamma ray burst 990123 (23 January 1999) was one of the brightest bursts recorded at the time, and was the first GRB with an optical ...More: http: //booksllc.net/?id=54342


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Product Details
  • ISBN-13: 9781158306602
  • Publisher: Books LLC
  • Publisher Imprint: Books LLC
  • Height: 152 mm
  • No of Pages: 26
  • Spine Width: 2 mm
  • Weight: 50 gr
  • ISBN-10: 1158306601
  • Publisher Date: 15 Sep 2010
  • Binding: Paperback
  • Language: English
  • Returnable: N
  • Sub Title: Energetic Gamma Ray Experiment Telescope, Grb 990123, 3c 279
  • Width: 229 mm


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