Characterization of clasts in the Glen Torridon region of Gale crater observed by the Mars Science Laboratory Curiosity Rover
Name
JGR Planets - 2022 - Khan - Characterization of Clasts in the Glen Torridon Region of Gale Crater Observed by the Mars.pdf
Description
Published version
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2.46 MB
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Adobe PDF
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Author(s) • • •
Khan, Sabrina
Stack, Kathryn M
Yingst, R Aileen
Bergmann, Kristin
Date Issued
2022
Journal
Journal of Geophysical Research: Planets
Publisher
American Geophysical Union (AGU)
Citation
Khan, Sabrina, Stack, Kathryn M, Yingst, R Aileen and Bergmann, Kristin. 2022. "Characterization of clasts in the Glen Torridon region of Gale crater observed by the Mars Science Laboratory Curiosity Rover." Journal of Geophysical Research: Planets, 127 (11).
Version
Final published version
Abstract
The morphology and composition of clasts have the potential to reveal the nature and extent of erosional processes acting in a region. Dense accumulations of granule- to pebble-sized clasts covering the ground throughout the Glen Torridon region of Gale crater on Mars were studied using data acquired by the Mars Science Laboratory Curiosity rover between sols 2300 and 2593. In this study, measurements of shape, size, texture, and elemental abundance of unconsolidated granules and pebbles within northern Glen Torridon were compiled. Nine primary clast types were identified through stepwise hierarchical clustering, all of which are sedimentary and can be compositionally linked to local bedrock, suggesting relatively short transport distances. Several clast types display features associated with fragmentation along bedding planes and existing cracks in bedrock. These results indicate that Glen Torridon clasts are primarily the product of in-situ physical weathering of local bedrock.
MIT Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
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Creative Commons Attribution NonCommercial License 4.0
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DOI of Published Version
https://doi.org/10.1029/2021JE007095