Instrument Information |
|
IDENTIFIER | urn:nasa:pds:context:instrument:fuvs.a17c::1.0 |
NAME |
APOLLO 17 FAR-ULTRAVIOLET SPECTROMETER (FUVS) |
TYPE |
SPECTROMETER |
DESCRIPTION |
Apollo 17 Far-Ultraviolet Spectrometer (FUVS), carried on board the Command and Servicing Module, measured the radiation intensity as a function of wavelength from 1180 to 1680 Angstrom. The prime objective of the scanning spectrometer was to measure the composition of the lunar atmosphere from orbit. Other observations included the lunar surface, zodiacal light, solar atmosphere emissions, earth emissions, and galactic and stellar emissions. |
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NAIF INSTRUMENT IDENTIFIER | |
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REFERENCES |
Apollo 17 Preliminary Science Report, NASA SP-330, published by NASA, Washington, D.C., 1973. Apollo Scientific Experiments Data Handbook, NASA Technical Memorandum X-58131, JSC-09166, published by NASA Johnson Space Center, Houston, Texas, Aug. 1974. Fastie, W.M.G., Apollo 17 far ultraviolet spectrometer experiment, The Moon, 7, 49-62, 1973. Fastie, W.G., P.D. Feldman, R.C. Henry, H.W. Moos, C.A. Barth, G.E. Thomas, T.M. Donahue, Search for far ultraviolet emissions from the lunar atmosphere, Science, 182, 710-711, 1973. Fastie, W.G., Final Report - Apollo 17 ultraviolet spectrometer experiment (S-169), Department of Physics, The Johns Hopkins University, NASA-CR-140316, Baltimore, MD, July 1974. |