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Elysium region, Mars - Tests of lithospheric loading models for the formation of tectonic featuresThe hypothesis that the tectonic features in the Elysium region are the product of stress produced by loading of the Martian lithosphere is tested. The lithospheric loading models for the formation of tectonic features in the Elysium region are evaluated under local loading, regional loading of the lithosphere from above and below, and quasi-global loading by Tharsis. The physiographic features in the Elysium region are described. The stress fields predicted by volcanic loading and uplift of the Martian lithosphere are compared with the tectonic features in the Elysium region. It is noted that the comparison suggests the succession of stress fields operating at different times in the region and supports the hypothesis.
Document ID
19870033572
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hall, J. Lynn
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Solomon, Sean C.
(MIT Cambridge, MA, United States)
Head, James W.
(Brown University Providence, RI, United States)
Date Acquired
August 13, 2013
Publication Date
October 1, 1986
Publication Information
Publication: Journal of Geophysical Research
Volume: 91
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
87A20846
Funding Number(s)
CONTRACT_GRANT: NSG-7297
CONTRACT_GRANT: NGR-40-002-116
Distribution Limits
Public
Copyright
Other

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