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The geology of the Viking Lander 2 siteModels are discussed of several competitive geologic histories that can be hypothesized for the Viking Lander 2 site, none of which is uniquely persuasive. The craft landed on a flat plain of fine-grained sediment overlain by dispersed evenly distributed boulders. The fine-grain material appears to be part of a high-latitude mantle comprising material swept south of the pole regions. The boulders, which are covered by distinctive deep pits, or vesicles, may be the residue of an ejecta deposit from the crater Mie. Alternatively, they may be the remnants of lava flows which formerly covered the region. Polygonal sediment-filled cracks may have been formed by ice wedging, similar to the process that occurs in terrestrial permafrost regions. The possibility that they are desiccation polygons may not be excluded.
Document ID
19780027527
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mutch, T. A.
(Brown University Providence, R.I., United States)
Arvidson, R. E.
(Brown Univ. Providence, RI, United States)
Guinness, E. A.
(Washington University St. Louis, Mo., United States)
Binder, A. B.
(Kiel, Universitaet Kiel, Germany)
Morris, E. C.
(U.S. Geological Survey, Branch of Astrogeologic Studies, Flagstaff Ariz., United States)
Date Acquired
August 9, 2013
Publication Date
September 30, 1977
Publication Information
Publication: Journal of Geophysical Research
Volume: 82
Subject Category
Lunar And Planetary Exploration
Accession Number
78A11436
Funding Number(s)
CONTRACT_GRANT: NASA ORDER L-9718
CONTRACT_GRANT: NAS1-9680
CONTRACT_GRANT: NAS1-13889
CONTRACT_GRANT: NAS1-11851
Distribution Limits
Public
Copyright
Other

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