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The puzzling moons of MarsViking Orbiter observations of Phobos and Deimos are presented with attention to physical dimension and surface features. Both satellites are approximately 1.4 times as long as they are wide; Phobos having a length of 27 km, while Deimos is half that size. In addition, both satellites are tidally locked, as is earth's moon, and are held together by cohesive forces as well as by gravity. Phobos and Deimos are both heavily cratered, and Phobos has deep (30 m) grooves in the vicinity of its largest crater, Stickney; indicating surface fracturing under meteorite impact. The craters on Deimos are largely filled with a fine-grained substance, probably crater ejecta.
Document ID
19780063340
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Veverka, J.
(Cornell Univ. Ithaca, NY, United States)
Thomas, P.
(Cornell University Ithaca, N.Y., United States)
Duxbury, T.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 9, 2013
Publication Date
September 1, 1978
Publication Information
Publication: Sky and Telescope
Volume: 56
Subject Category
Lunar And Planetary Exploration
Accession Number
78A47249
Distribution Limits
Public
Copyright
Other

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