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Geomorphic evidence for ancient seas in west Deuteronilus Mensae, Mars-1: Regional geomorphologyThe fretted terrain in west Deuteronilus Mensae consists of extensive cratered upland penninsulas or isolated plateaus cut by long, finger-like canyons typically 10 to 20 km wide and upwards of 300 km long. The longest of these canyons trend roughly north-south to north-northeast, which may reflect some local structural and/or topographic control. At least three geomorphic zones roughly parallel to the lowland/upland boundary, suggestive of increasing modification northward, can be recognized on the fretted region of the region. The southern-most zone (zone A) consists of sharply defined fretted terrain. The middle zone (zone B) consists of well defined fretted terrain in which the plateau surfaces appear smoother, with a somewhat darker and much less varied albedo surface than those of zone A. The northern-most zone (zone C) consists of rounded or softened fretted terrain. The zones were interpreted as surface exposures of successively lower stratigraphic units.
Document ID
19870014038
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Parker, Timothy J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Schneeberger, Dale M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Pieri, David C.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Saunders, R. Stephen
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 5, 2013
Publication Date
May 1, 1987
Publication Information
Publication: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986
Subject Category
Lunar And Planetary Exploration
Accession Number
87N23471
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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