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The Martian satellites - 100 years onStudies of Phobos and Deimos, the two satellites of Mars, may provide the best observations yet of the material populating the asteroid belt. Viking observations of Phobos showing crater chains and striations are analyzed, and Mariner-9 photometry exhibiting the albedo of the satellite is discussed. A mass determination for Phobos results in a value of 1.1 times 10 to the 19th power g; the mean density of the satellite is set at about 2 g per cu cm, a value suggesting formation of the satellite from material in the asteroid belt.
Document ID
19780052520
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hunt, G. E.
(University College London, United Kingdom)
Michael, W. H., Jr.
(NASA Langley Research Center Hampton, Va., United States)
Pascu, D.
(U.S. Naval Observatory Washington, D.C., United States)
Veverka, J.
(Cornell University Ithaca, N.Y., United States)
Wilkins, G. A.
(Royal Greenwich Observatory Herstmonceux, Sussex, United Kingdom)
Woolfson, M.
(York, University Heslington, United Kingdom)
Date Acquired
August 9, 2013
Publication Date
March 1, 1978
Publication Information
Publication: Royal Astronomical Society
Subject Category
Lunar And Planetary Exploration
Accession Number
78A36429
Distribution Limits
Public
Copyright
Other

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