- OSO 3
OSO 3 Operator NASA Major contractors Ball Brothers Research Corporation (BBRC) Mission type Solar Physics Satellite of Earth Launch date March 8, 1967 at 16:19:00 UTC Launch vehicle Thor-Delta Launch site Cape Canaveral, United States Mission duration 2 yr 8 mn COSPAR ID 1967-020A Mass 281 kg Orbital elements Eccentricity 0.002164 Inclination 32.87° Altitude 550 km Apoapsis 464.0 km Periapsis 534.0 km Orbital period 95.53 min. Orbits per day 15.07
OSO 3, third Orbiting Solar Observatory (known as OSO C before launch) was launched on March 8, 1967, into a nearly circular orbit of mean altitude 550 km, inclined at 33° to the equatorial plane. Its on-board tape recorder failed on June 28, 1968, allowing only the acquisition of sparse real-time data during station passes thereafter; the last data were received on November 10, 1969. OSO 3 reentered the Earth's atmosphere and burned up on April 4, 1982.
Like all the American OSO-series satellites, it had two major segments: one, the "Sail", was stabilized to face the Sun, and carried both solar panels and Sun-pointing experiments for solar physics. The other, "Wheel" section, rotated to provide overall gyroscopic stability and also carried sky scanning instruments that swept the sky as the wheel turned, approximately every 2 sec.
Experiments on board OSO 3 Name Target Principal Investigator High Energy Gamma Ray (> 50 MeV) anti-solar Kraushaar, W. L., Massachusetts Institute of Technology Cosmic Ray Spectrum Detector and Gamma Ray Analyzer Sun, all-sky Kaplon, Morton F, University of Rochester Directional Radiometer Experiment Earth Neel, Carr B Jr, NASA Ames Research Center Earth Albedo (0.32- to 0.78-µm) Earth Neel, Carr B Jr, NASA Ames Research Center Solar EUV Spectrometer 0.1 to 40.0 nm Sun Neupert, Werner M, NASA Goddard Space Flight Center 0.8- to 1.2-nm Solar X-Ray Ion Chamber Sun Teske, Richard G, University of Michigan Solar and Celestial Gamma-Ray Telescope (7.7 to 200 keV) Sun, all-sky Peterson, Laurence E, University of California, San Diego Thermal Radiation Emissivity near-Earth space environment Neel, Carr B Jr, NASA Ames Research Center Extreme Ultraviolet Spectrometer Sun Hinteregger, Hans E, Phillips Laboratory
The Sail carried a hard X-ray experiment from UCSD, with a single thin NaI(Tl) scintillation crystal plus phototube enclosed in a howitzer-shaped CsI(Tl) anti-coincidence shield. The energy resolution was 45% at 30 keV. The instrument operated from 7.7 to 210 keV with 6 channels. The Principal Investigator (PI) was Prof. Laurence E. Peterson of UCSD. Also in the wheel was a cosmic gamma-ray (>50 MeV) sky survey instrument contributed by MIT, with PI Prof. William L. Kraushaar].
OSO-3 obtained extensive observations of solar flares, the cosmic diffuse X-ray background, and the observation of a single flare episode from Scorpius X-1, the first observation of an extrasolar X-ray source by an observatory satellite. The MIT gamma-ray instrument obtained the first identification of high-energy cosmic gamma rays emanating from both galactic and extra-galactic sources.
- ^ NASA GSFC X-ray Astronomy Satellites and Missions
- ^  GSFC HEASARC "The Third Orbiting Solar Observatory (OSO-3)"
- ^ Pelling, R. M. 1971, Ph.D. dissertation thesis, University of California at San Diego,
- ^ Peterson et al 1966, Phys Rev Let 16, 142,
- ^ Peterson et al 1966, ApJ 145, 962.
- ^ Kraushaar, W. L., G. W. Clark, G. P. Garmire, R. Borken, P. Higbie, V. Leong, and T. Thorsos. 1972. High-energy cosmic gamma-ray observations from the OSO-3 satellite. Ap.J. 177: 341-363.ADS
Solar space observatory missions Current Future Completed On hiatus Cancelled
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