T84 Geomorphology and Landscape Evolution of Mars
Monday, 16 October 2023
8:00 AM - 12:00 PM
323
DECIPHERING MARS' GLOBAL ATMOSPHERE THROUGH THE LENS OF BARCHAN DUNE MORPHOLOGY
Paper number: T84-12
Program: Technical Sessions
Time: 10:40 AM – 11:00 AM
Authors
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Mathieu LapotreStanford UniversityGeological Sciences, Stanford, CA
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Andrew GunnMonash University, Melbourne
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Ryan C. EwingTexas A&M, College Station, TX
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Lori FentonSETI Institute, Mountain View, CA
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Matthew ChojnackiPlanetary Science Institute, Tucson, AZ
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Alejandro SotoSouthwest Research Institute, Boulder, CO
Abstract
Our study opens several new avenues for understanding Mars' atmosphere and the physical laws that govern aeolian sand transport; the correlation between the sizes of incipient dunes and atmospheric density sheds light on the hydrodynamic principles controlling the formation of large martian ripples. The orientations of barchan slipfaces, which predominantly align with the primary wind direction, provides a detailed picture of wind circulation across the Martian surface. The changing dynamics of dune slipfaces in volatile-rich environments reveal how aeolian sand transport responds to the presence of surface and ground ice. These findings underscore the importance of global geomorphological investigations, especially those aided by machine learning techniques, in advancing our understanding of planetary climates and physics-based theory in extraterrestrial environments.
Geological Society of America Abstracts with Programs. Vol. 55, No. 6
doi: 10.1130/abs/2023AM-388903
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