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Mariner 9 television observations of Phobos and Deimos.Mariner 9 photographs of Phobos and Deimos have yielded new information about the orbits, rotation periods, sizes, shapes, and surface characteristics of the satellites. Both satellites appear to be in synchronous rotation. They are irregular, heavily cratered bodies whose shapes appear to have been determined largely by impact fragmentation and spalling. The surfaces of both satellites have crater densities close to saturation and nearly identical, very low albedos. Lower limits on the tensile and yield strengths are estimated, and it is concluded that both satellites may consist of well-consolidated, though possibly highly fractured material.
Document ID
19730032678
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Pollack, J. B.
(NASA Ames Research Center Moffett Field, Calif., United States)
Veverka, J.
Noland, M.
Sagan, C.
(Cornell University Ithaca, N.Y., United States)
Hartmann, W. K.
(Science Applications, Inc. Tucson, Ariz., United States)
Duxbury, T. C.
Born, G. H.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Milton, D. J.
(U.S. Geological Survey Menlo Park, Calif., United States)
Smith, B. A.
(New Mexico State University Las Cruces, N. Mex., United States)
Date Acquired
August 7, 2013
Publication Date
October 1, 1972
Subject Category
Space Sciences
Accession Number
73A17480
Distribution Limits
Public
Copyright
Other

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