T113 Best Practices and Exciting Discoveries in Identifying, Mapping, and Analyzing Planetary Landforms and Terrestrial Analogues (Posters)
Monday, 16 October 2023
8:00 AM - 5:30 PM
Hall B
DISTRIBUTION OF BOULDERS AROUND DE GERLACHE CRATER AND LUNAR SOUTH POLE CANDIDATE LANDING REGIONS
Paper number: T113-2
Program: Technical Sessions
Time: 8:00 AM – 5:30 PM
Authors
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Isaac L. HollingsworthTennessee Tech University, Cookeville, TN
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Jeannette LunaTennessee Tech University, Cookeville, TN
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Philip RobersonTennessee Tech University, Cookeville, TN
Abstract
Here, we present a map of >10,000 boulders occurring as: (1) distal isolated blocks as well as (2) boulder fields. Our mapping is based on data returned from the Lunar Reconnaissance Orbiter (LRO) mission. Where possible and practical, we used Narrow Angle Camera (NAC) photomosaics to identify geologic units and boulders. In areas with significant shadow, we relied on Lunar Orbiter Laser Altimeter (LOLA) high-resolution digital elevation models and hillshades to estimate the boundaries of boulder fields or individual clusters. Approximately 94.91% of boulders in the de Gerlache area rest on slopes less than the angle of repose, 30 degrees; 57.02% rest on slopes accessible by humans or robotic rovers, 20 degrees. It is likely that many of these boulders are older than 3.85 Ga, and thus represent some of the oldest crustal material accessible in the Solar System. As a result of this work, we document areas where boulder fields occur on very old crust adjacent to known volatiles or permanently shadowed regions, areas that thus meet many of the high priority objectives of upcoming Artemis missions.
Geological Society of America Abstracts with Programs. Vol. 55, No. 6
doi: 10.1130/abs/2023AM-392864
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