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- W4224303546 endingPage "1887" @default.
- W4224303546 startingPage "1887" @default.
- W4224303546 abstract "The presence of buried glacial ice and putative extinct rock glaciers in Mars’ equatorial regions has implications for understanding its climate history and sensitivity to changes in insolation and has significant implications for past global redistribution of the water ice cryosphere. We quantify the morphology of rock glacier- “like” features on the northern slopes of Aeolis Mons (known also as Mount Sharp) within Gale crater and use this information to evaluate a possible rock glacier origin for these forms. Detailed morphometric evaluation of cross and long profiles of these lobate features, which exhibit higher slopes at their heads, lower slopes at their distal edge, and a convex upward cross-sectional profile and oversteepened sides, resembles active terrestrial rock glaciers. However, the absence of a chevron wrinkle pattern and sublimation features could indicate extensive aeolian reworking and the lack of deflation could indicate a higher rock to ice mixture. The lack of cratering surfaces relative to the cratered surfaces that they overly could indicate a younger age and are possibly indistinguishable in age from the capping units of Mount Sharp, which may have once been more laterally extensive and may have been the source of these mass wasting forms." @default.
- W4224303546 created "2022-04-26" @default.
- W4224303546 creator A5017595739 @default.
- W4224303546 creator A5038533444 @default.
- W4224303546 creator A5073504754 @default.
- W4224303546 date "2022-04-14" @default.
- W4224303546 modified "2023-10-03" @default.
- W4224303546 title "Numerical Analysis of Putative Rock Glaciers on Mount Sharp, Gale Crater, Mars" @default.
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