T264 Latest Science Results and Updates in Planetary Science Research, Programs and Flight Projects
Wednesday, 18 October 2023
1:30 PM - 5:30 PM
323
RIMFAX GROUND PENETRATING RADAR OBSERVATIONS OF THE WESTERN FAN, JEZERO CRATER, MARS
Paper number: T264-6
Program: Technical Sessions
Time: 2:50 PM – 3:05 PM
Authors
-
Svein-Erik HamranKjeller
-
David PaigeUniversity of California, Los Angeles, Los Angeles, CA
-
Hans E.F. AmundsenInstitute for Technology Systems, Kjeller
-
Tor BergerKjeller
-
Titus CasademontKjeller
Abstract
The fan is confirmed to be younger than surrounding (likely igneous) crater floor materials, with the latter diving beneath onlapping sediments of the fan in the Cape Nukshak section. The relationship is more complex at the very toe of the Hawksbill Gap section, though the fan-crater floor interface is fairly flat and distinct in the more fanwards subsusrface. The stack of layers exposed in the fan front up to Hogwallow Flats are nearly horizontal. In contrast, Rockytop and higher materials slope downwards towards the fan edge, indicating a different episode of emplacement. Within the curvilinear Tenby Formation, steep dips and truncations of layer sets are apparent in select profile sections, allowing the intricate relationships of curvilinear surface sets to be extended to the subsurface. A likely broad erosional trough is apparent high in the Tenby Formation (beneath Emerald Lake), and potential evidence for buried narrower rilles may also exist. Parts of the subsurface here appear relatively featureless, especially where the upper near-surface is highly scattering, likely due to high concentrations of cobbles and boulders that are seen covering neighboring areas of the surface. RIMFAX subsurface GPR results have significantly augmented and illuminated more traditional rover surface observations, in a fundamentally new way over previous Mars rover missions.
Geological Society of America Abstracts with Programs. Vol. 55, No. 6
doi: 10.1130/abs/2023AM-394275
© Copyright 2023 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.