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Geological framework of the south polar region of Mars.The first 4 months of Mariner 9 photography of the south polar region are discussed. Three major geological units have been recognized, separated by erosional unconformities. From oldest to youngest they are: cratered terrain, pitted plains, and laminated terrain. The latter unit is unique in occurrence to the polar region, volatiles are probably involved in its origin, and may still be present within the laminated terrain as layered ice. The residual south polar cap has been observed to survive the disappearance of the thin annual CO2 frost deposit and to last virtually unchanged in outline through the southern summer. That exposed deposit is inferred to be composed of water-ice. The residual cap appears to lie at the apex of an unusual quasi-circular structure composed of laminated terrain; a similar structure also appears to exist near the north pole.
Document ID
19730032675
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Murray, B. C.
Sharp, R. P.
Leighton, R. B.
(California Institute of Technology Pasadena, Calif., United States)
Soderblom, L. A.
(California Institute of Technology, Pasadena, Calif.; U.S. Geological Survey, Astrogeology Branch, Flagstaff Ariz., United States)
Cutts, J. A.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Milton, D. J.
(U.S. Geological Survey, Astrogeology Branch, Menlo Park Calif., United States)
Date Acquired
August 7, 2013
Publication Date
October 1, 1972
Subject Category
Space Sciences
Accession Number
73A17477
Distribution Limits
Public
Copyright
Other

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