Einstein Observatory
Einstein Observatory (HEAO-2) was the first fully imaging X-ray telescope put into space and the second of NASA's three High Energy Astrophysical Observatories. Named HEAO B before launch, the observatory's name was changed to honor Albert Einstein upon its successfully attaining orbit.[1]
Einstein Observatory | |
Mission type | Astronomy |
---|---|
Operator | NASA |
COSPAR ID | 1978-103A |
SATCAT no. | 11101 |
Website | Einstein Observatory at NASA.gov |
Mission duration | 4 years |
Spacecraft properties | |
Manufacturer | TRW |
Dry mass | 3,130 kilograms (6,900 lb) |
Start of mission | |
Launch date | 13 November 1978, 05:24 UTC |
Rocket | Atlas SLV-3D Centaur-D1AR |
Launch site | Cape Canaveral LC-36B |
End of mission | |
Last contact | 17 April 1981 |
Decay date | 26 May 1982 |
Orbital parameters | |
Reference system | Geocentric |
Regime | Low Earth |
Perigee altitude | 465 kilometres (289 mi) |
Apogee altitude | 476 kilometres (296 mi) |
Inclination | 23.5° |
Period | 94.0 minutes |
Epoch | 13 November, 1978 05:24:00 UTC |
Launch
The Einstein Observatory, HEAO-2, was launched on November 13, 1978, from Cape Canaveral, Florida, on an Atlas-Centaur SLV-3D booster rocket into a near-circular orbit with an initial altitude slightly above 500 km. Its orbital inclination orbit was 23.5 degrees. The Einstein Observatory satellite re-entered the Earth's atmosphere and burned up on March 25, 1982.[2]
Instrumentation
The Einstein Observatory carried a single large grazing-incidence focusing X-ray telescope that provided unprecedented levels of sensitivity (hundreds of times better than previously achieved) and arc-second angular resolution of point sources and extended objects. It had instruments sensitive in the 0.2 to 3.5 keV energy range. A collection of four focal-plane instruments was installed in the satellite: [3]
- HRI, or High Resolution Imaging camera, 0.15-3 keV
- IPC, or Imaging Proportional Counter, 0.4 to 4 keV
- SSS, or Solid State Spectrometer, 0.5 to 4.5 keV
- FPCS, or Bragg Focal Plane Crystal Spectrometer
There was also a coaxial instrument 'MPC', the Monitor Proportional Counter, working in the 1-20 keV range, and two filters that could be used with the imaging detectors:
- BBFS, Broad Band Filter Spectrometer (aluminium and beryllium filters than can be placed into the X-ray beam, to change the spectral sensitivity)
- OGS, Objective grating spectrometer (transmission gratings with a spectral resolution of about 50)
References
- "HEA Heritage Missions: Einstein Observatory". cfa.harvard.edu. Retrieved March 27, 2014.
- "Einstein Observatory (HEAO-2)". ecuip.lib.uchicago.edu. Retrieved March 27, 2014.
- "The Einstein /HEAO 2/ X-ray Observatory". adsabs.harvard.edu. Retrieved March 27, 2014.
See also
Wikimedia Commons has media related to HEAO 2. |