The High Energy Astronomy Observatory Program was a NASA program of the late 1970s and early 1980s that included a series of three large low-Earth-orbiting spacecraft for X-ray and Gamma-Ray astronomy and Cosmic-Ray investigations. After launch, they were denoted HEAO 1, HEAO 2 (also known as The Einstein Observatory), and HEAO 3, respectively. The first of NASA's three High Energy Astronomy Observatories HEAO 1, launched August 12 1977 aboard an Atlas rocket with a Centaur upper stage operated 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 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 The last of NASA's three High Energy Astronomy Observatories, HEAO 3 was launched 20 September 1979 on an Atlas-Centaur launch The large (~3000 kg) spacecraft were 3-axis stabilized to arc-minute accuracy, with fixed solar panels. All were launched from Cape Canaveral on Atlas/Centaur SLV-3D lunch vehicles into near-circular orbits with initial altitudes slightly above 500 km.
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HEAO 1, launched August 12, 1977, was a sky survey mission that included four large X-ray and gamma-ray astronomy instruments, known as A1, A2, A3, and A4, respectively. The first of NASA's three High Energy Astronomy Observatories HEAO 1, launched August 12 1977 aboard an Atlas rocket with a Centaur upper stage operated Inclination was about 22. 7 degrees. It re-entered 15 March, 1979.
HEAO 2, more commonly known as the Einstein Observatory, launched 13 November, 1978 into a 23. 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 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 5 deg inclination orbit, carried a single large grazing-incidence focusing X-ray telescope, providing unprecedented levels of sensitivity (hundreds of times better than previously achieved) and arc-second angular resolution for pointed observations of known objects, and operated over the 0. 2 to 3. 5 keV energy range. A suite of four focal plane instruments were provided:
as well as a 1-20 keV Monitor Proportional Counter (MPC), a Broad Band Filter Spectrometer (BBFS), and an objective grating spectrometer (OGS). The spacecraft re-entered 25 March, 1982.
HEAO 3, launched on 20 September 1979 into a 43. The last of NASA's three High Energy Astronomy Observatories, HEAO 3 was launched 20 September 1979 on an Atlas-Centaur launch 6-degree inclination orbit, carried three experiments, known as C1, C2, and C3. The first was a cryogenically cooled germanium (Ge) high-resolution gamma-ray spectrometer, while the C2 and C3 experiments were large cosmic-ray instruments. A spectrometer is an Optical instrument used to measure properties of Light over a specific portion of the Electromagnetic spectrum, typically used For the 1962 Bruce Conner film see Cosmic Ray (film Cosmic rays are energetic particles originating from space that impinge on Re-entry was 7 December, 1981.
The experiment designations A1, A2, A3, A4, for HEAO A, thru C1, C2, C3 for HEAO C, were most common before launch, but also often appear in the later scientific literature. The first of NASA's three High Energy Astronomy Observatories HEAO 1, launched August 12 1977 aboard an Atlas rocket with a Centaur upper stage operated The last of NASA's three High Energy Astronomy Observatories, HEAO 3 was launched 20 September 1979 on an Atlas-Centaur launch The overall HEAO program was managed out of NASA's Marshall Space Flight Center in Huntsville, AL. NASA Program Manager was Mr. Richard E. Halpern; NASA Program Scientist was Dr. Albert G. Opp. Total program cost was roughly $250 million[1].