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Orbiting Astronomical Observatory 3
Copernicus or OAO-3 (Orbiting Astronomical Observatory 3), also mentioned as Orbiting Astronomical Observatory-C,[1][2] was a space telescope intended for ultraviolet and X-ray observation. After its launch, it was named Copernicus to mark the 500th anniversary of the birth of Nicolaus Copernicus in 1473. Part of the Orbiting Astronomical Observatory program, it was a collaborative effort between NASA and the UK's Science Research Council (currently known as the Science and Engineering Research Council).[3] Copernicus collected high-resolution spectra of hundreds of stars, galaxies and planets, remaining in service until February 1981.[1] HistoryThe OAO-3 satellite, weighing 2,150 kg, was launched on August 21, 1972, by an Atlas SLV-3C from Launch Complex 36, Cape Canaveral, Florida.[4] The mission used a new inertial reference unit that was developed by the Massachusetts Institute of Technology.[5] Between 1972 and February 1981,[4] it returned high-resolution spectra of 551 stars along with extensive X-ray observations.[6] Among the significant discoveries made by Copernicus were the discovery of several long-period pulsars such as X Persei that had rotation times of many minutes instead of the more typical second or less, and confirmation that most of the hydrogen in interstellar gas clouds existed in molecular form.[5] InstrumentationCopernicus carried two instruments:[5]
See alsoReferences
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