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Tenma

Japanese space observatory (1983–1988) From Wikipedia, the free encyclopedia

Tenma
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Tenma, known as ASTRO-B before launch, was a Japanese X-ray astronomy satellite developed by the Institute of Space and Astronautical Science. It was launched on 20 February 1983, using a M-3S rocket on the M-3S-3 mission. It was the second X-ray observatory successfully operated by Japan after Hakucho (CORSA-B),[3][a] and it had a superior temporal and spectral sensitivity compared to its predecessor.[5]

Quick facts Names, Mission type ...

Battery failure in July 1984 caused the operation to become limited, and continuing problems lead to the termination of X-ray observation on 11 November 1985,[6] however it remained in sporadic contact until 17 December 1988.[2] It reentered the atmosphere on 19 January 1989.[b]

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Highlights

  • Discovery of the iron helium-like emission from the galactic ridge.[6]
  • Iron line discovery and/or study in many LMXRB, HMXRB and AGN.[2]
  • Discovery of an absorption line at 4 keV in the X1636-536 Burst spectra.

References

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