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Chaotic terrain of Mars - A tectonic interpretation from Mariner 6 imagerySharp et al. (1971) define chaotic terrain as an irregular jumble of topographic forms covering a certain area within Pyrrhae Regio and adjacent regions centered at about 10 deg S., 35 deg W. This area is covered by Mariner 6 television imagery. An analysis of fracture patterns in the Martian surface from high-resolution Mariner 6 imagery suggests that the lineaments observed in both the chaotic terrain and the cratered plateau areas in Pyrrhae Regio are tectonic fractures resulting from stresses within the Martian crust.
Document ID
19740048679
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wilson, R. C.
Harp, E. L.
Picard, M. D.
Ward, S. H.
(Utah, University Salt Lake City, Utah, United States)
Date Acquired
August 7, 2013
Publication Date
March 1, 1973
Publication Information
Publication: Geological Society of America Bulletin
Volume: 84
Subject Category
Space Sciences
Accession Number
74A31429
Funding Number(s)
CONTRACT_GRANT: NGR-45-003-085
Distribution Limits
Public
Copyright
Other

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