237 Geomorphology and Surface Processes Across the Solar System
This session welcomes abstracts on any aspect of planetary geomorphology and surface processes, including but not restricted to: Earth analogues, laboratory experiments, numerical models, planetary comparison, mapping, in situ data, or remote sensing studies.
Wednesday, 22 October 2025
8:00 AM - 12:00 PM
HBGCC, 212AB
Global distribution of martian sedimentary basins
Paper number: 237-6
Program: Technical Sessions
Time: 9:30 AM – 9:45 AM
Authors
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Timothy GoudgeUniversity of Texas at Austin, Austin
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David MohrigThe University of Texas at Austin, Geological Sciences, Austin, TX
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Benjamin CardenasPenn State, University Park, PA
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Mackenzie DayUniversity of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA
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Kathryn Stack MorganJet Propulsion Laboratory, Pasadena, CA
Abstract
Layered sedimentary deposits compose thousands of outcrops across the martian surface, preserving one of the planet’s most complete records of past climate and habitability. Yet whether these sediments accumulated within discrete, long‑lived basins—analogous to terrestrial sedimentary basins—or were merely distributed, patchy outcrops remains unresolved. Here we synthesize ~22 000 published and unpublished observations from sediment-bearing landforms, including stratified deposits, fan-shaped bodies, paleo-bedforms, fluvial depositional ridges and sedimentary mounds to establish their spatial relationship to martian topography. The inventory reveals those sedimentary accumulations cluster geographically within major sinks such as the Northern Lowlands, Hellas, Valles Marineris, Meridiani Planum and the Medusae Fossae Formation. Analysis of topographic parameters—elevation and the Topographic Position Index (TPI), which classifies landscape features by their elevation relative to surrounding terrain—shows that these deposits occupy long‑wavelength accommodation space, with erosional valley networks are preferentially situated upslope. This systematic arrangement on the martian landscape leads us to hypothesize that these hot spots of sedimentary deposits represent the modern expression of large, persistent sedimentary basins that formed on early Mars. Ongoing work to potentially quantify the thickness, areal extent and volume of these basins will provide critical constraints on models of surface processes, climate evolution and the planet’s potential for sustaining life.
Geological Society of America Abstracts with Programs. Vol. 57, No. 6
doi: 10.1130/abs/2025AM-414384
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