T138 Geomorphology and Landscape Evolution of Mars
Monday, 5 November 2018
1:30 PM - 5:30 PM
Room 236-237
EXTENT AND TIMING OF HYDROLOGIC ACTIVITY IN THE GALE CRATER REGION OF MARS
Paper number: T138-5
Program: Technical Sessions
Time: 2:40 PM – 3:00 PM
Authors
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Melanie KanineDartmouth College, Hanover, NH
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Frances Rivera-HernandezDartmouth College, Hanover, NH
Abstract
We investigated 24 candidate deltaic landforms, twelve of which have been characterized in previous studies. Deltas were differentiated from other depositional features, such as alluvial fans and landslide deposits, based on their arcuate form, low-gradient tops, and steeply-dipping fronts. They also tended to originate from short, stubby, v-shaped valleys with amphitheater-shaped terminations. Delta front elevations were found to vary by ~2620 m, ranging from -3980 m to -1360 m. The deltaic deposits were rarely isolated, rather they typically were clustered in groups of 2 to 5 deltas. In each of these groups the deltas generally had similar front elevations to one another; within ~30 to 200 m range. Using delta front elevations as water level proxies, we found evidence for several distinct enclosed basins into which these features formed. We also performed crater counting on these features, as well as the basins into which they likely formed. While several of these deltas did not correspond to an enclosed basin, these data suggest that most dichotomy deltas in the Gale region record large lakes, not a global ocean, which has significant implications for the timing and size of Mars’ past global hydrosphere.
Geological Society of America Abstracts with Programs. Vol. 50, No. 6
doi: 10.1130/abs/2018AM-319470
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