Quick Facts
| Mission Name |
OSO-8: Orbiting Solar Observatory-8
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| LASP Instruments |
High-Resolution Ultraviolet Spectrometer Measurements
Principal Investigator: Charles A Barth
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| Destination |
Approx 550 km Earth Orbit
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| Launch Date |
June 21st, 1975
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| Launch Location |
Kennedy Space Center
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| Launch Vehicle |
Delta
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| Mission Duration |
3 1/3 years
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Mission Description/
LASP involvement |
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| LASP Divisions Involved |
Science
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| LASP Mission Web Page |
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| Official Mission Web Page |
http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=1975-057A
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The Science and Goal
The objectives of the OSO satellite series were to perform solar physics experiments above the atmosphere during a complete solar cycle and to map the entire celestial sphere for direction and intensity of UV light, X-ray radiation, and gamma-ray radiation. The OSO 8 platform consisted of a sail section, which pointed two experiments continually toward the sun, and a wheel section, which spun about an axis perpendicular to the pointing direction of the sail and carried five experiments. Gas jets and a magnetic torquing coil performed attitude adjustment. Pointing control permitted the pointed experiments to scan the region of the solar disk in a 40- by 40-arc-min to 60- by 60-arc-min raster pattern. In addition, the pointed section was capable of being commanded to select and scan a 1- by 1-arc-min or 5- by 5-arc-min region anywhere on the solar disk. Data were simultaneously recorded on tape and transmitted by PCM/PM telemetry. A command system provided for at least 512 ground-based commands. For more information, see S. P. Maran and R. J. Thomas, Sky & Teles., v. 49, p. 355, 1975.
(This information taken from: http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=1975-057A)
No information available
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