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Evidence for an Ancient Buried Landscape on the NW Rim of Hellas Basin, MarsHellas basin is the largest (2000+ km across) well-preserved impact structure on Mars and its deepest depositional sink [e.g., 1]. The Hellas rim and adjacent highlands are of special interest given the possibility of paleolakes on the basin floor [2-4], recent studies of potential localized fluvial/lacustrine systems [2, 5-17], and evidence for phyllosilicates around and within impact craters north of the basin [18-26]. We are producing a 1:1.5M-scale geologic map of eight MTM quadrangles (-25312, -25307, -25302, -25297, -30312, -30307, -30302, -30297) along Hellas NW rim. The map region (22.5-32.5degS, 45- 65degE) includes a transect across the cratered highlands of Terra Sabaea, the degraded NW rim of Hellas, and basin interior deposits of NW Hellas Planitia. No previous mapping studies have focused on this region, although it has been included in earlier global and regional maps [27-29].
Document ID
20110002774
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Crown, David A.
(Planetary Science Inst. Tucson, AZ, United States)
Bleamaster, Leslie F., III
(Planetary Science Inst. Tucson, AZ, United States)
Mest, Scott C.
(Planetary Science Inst. Tucson, AZ, United States)
Mustard, John F.
(Brown Univ. Providence, RI, United States)
Vincendon, Mathieu
(Brown Univ. Providence, RI, United States)
Date Acquired
August 25, 2013
Publication Date
June 1, 2010
Publication Information
Publication: Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ, 2010
Subject Category
Geosciences (General)
Distribution Limits
Public
Copyright
Public Use Permitted.
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