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Published December 2022 | public
Journal Article

Barform deposits of the Carolyn Shoemaker formation, Gale crater, Mars

Abstract

The early environmental history of Mars is encoded in the planet's record of sedimentary rocks. Since 2012, the Curiosity rover has been ascending Mount Sharp, Gale crater's central mound, making detailed observations of sedimentary strata exposed there. The primary depositional setting represented by the rocks examined thus far has been a perennial lake, represented by the mudstones and sandstone lenses of the Murray formation. Here, we report on the sedimentology of outcrops examined in the Carolyn Shoemaker formation, which sits stratigraphically above the Murray formation. We interpret strata exposed in the Glasgow and Mercou members of the Carolyn Shoemaker formation to represent river bars in ancient alluvial and shoreline settings based on sedimentary structures, stratal geometries measured from photogrammetric data, and erosional morphology. The transition from a lacustrine to a fluvial depositional setting records the aggradation and progradation of coastal rivers into what was previously the extent of the Gale lake system. This may have occurred due to the shrinking of the lake over time due to climate-driven changes in the basin water balance, or local three-dimensionality in shoreline evolution, such as the formation of a new sedimentary lobe following a channel switch.

Additional Information

We would like to thank Journal of Sedimentary Research Editor Kathleen Marsaglia, Associate Editor John Gillies, and Technical Editor John Southard for the handling of our manuscript. Reviewers Ellen Chamberlin and Chenliang Wu are thanked for their thoughtful comments that helped improve the text and figures. We acknowledge Ashwin Vasavada and MSL science-team members and collaborators who participated in operations during these imaging campaigns, and members of the MSL Sedimentology and Stratigraphy Working Group for discussions. We thank the Malin Space Science Systems team for their efforts. BTC thanks Jay Dickson for assistance in Caltech's Murray Lab for Planetary Visualization, where the analysis was performed, as well as Tim Goudge, Hima Hassenruck-Gudipati, Cory Hughes, Joe Levy, Woong Mo Koo, David Mohrig, and Feifei Zhao for their work at the Morrison Formation between 2015 and 2018. GC was supported in France by French Agence Nationale de la Recherche (ANR) under the contract ANR-16-CE31-0012 entitled Mars-Prime, and by the French space agency CNES under convention CNES 180027. Data used in this manuscript are available at the Caltech Data Repository, http://dx.doi.org/10.22002/D1.20044.

Additional details

Created:
August 22, 2023
Modified:
October 23, 2023