Evolution of a Lake Margin Recorded in the Sutton Island Member of the Murray Formation, Gale Crater, Mars
Abstract
This study uses data from the Mars Science Laboratory Curiosity rover to document the facies of the Sutton Island member of the Murray formation, interpret paleoenvironments, and establish key stratigraphic transitions at Gale crater. Two facies associations were identified: Facies Association 1 (FA1) and Facies Association 2 (FA2). Individual facies in FA1 include planar-laminated mudstone with minor intervals of planar sandstone, ripple cross-laminated sandstone, cross-stratified sandstone, and alternating laminated sandstone and mudstone. Meter-thick packages of planar-laminated mudstone in FA1 are interpreted to represent deposition in low-energy ponded environments along the lake margin. Straight- and curve-crested ripple cross-laminated facies are interpreted to represent current-influenced deposition. Cross-stratified sandstone facies consist of dm-thick sets that represent deposition in distal channels. Intercalated mm-scale mudstone and sandstone laminae represent waning flow conditions and possible channel abandonment. Facies in FA1 collectively represent deposition in a distal delta plain. FA2 is comprised of planar-laminated mudstone with minor sandstone and is interpreted to represent deposition in a lacustrine-basin setting by suspension settling linked to density flows. FA1 transitions upward into FA2, defining a rapid transgression substantial enough to facilitate the deposition of distal lake facies above delta plain facies. The abrupt transition from FA2 back to FA1 deltaic deposits is suggestive of forced regression. Facies in FA1 and FA2 are consistent with the prevalence of aqueous environments recorded in other Murray formation members and extend our understanding of the dynamic sedimentary processes that characterized ancient lacustrine systems at Gale crater.
Copyright and License
© 2024 American Geophysical Union. This article has been contributed to by U.S. Government employees and their work is in the public domain in the USA.
Acknowledgement
The authors acknowledge the extensive efforts of the MSL Curiosity rover engineering and science operations teams as well as the MSL Sedimentology and Stratigraphy Working Group. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Mastcam mosaics were processed by the Mastcam team at Malin Space Science Systems. We thank Libby Ives and Michael Thorpe for the comprehensive reviews that greatly improved the quality of this manuscript. S. Gwizd and C. Fedo acknowledge funding from NASA/JPL subcontract #1546201.
Data Availability
The code repository for the MMGIS interface can be accessed through (https://github.com/NASA-AMMOS/MMGIS) and is detailed by Calef et al. (2019). The HiRISE mosaic used through the MMGIS interface can be accessed through Calef and Parker (2016). Data derived from HiRISE (McEwen, 2005) and CTX (Malin, 2007) images can also be accessed through the NASA Planetary Data System Geosciences Node (https://pds-geosciences.wustl.edu/missions/mro/default.htm). All Mastcam (Malin, 2013) and MAHLI (Edgett, 2013a, 2013b) images used in this manuscript may be accessed through the NASA Planetary Data System Cartography and Imaging Sciences Node (https://pds-imaging.jpl.nasa.gov/volumes/msl.html).
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Additional details
- ISSN
- 2169-9100
- Jet Propulsion Laboratory
- 1546201
- Caltech groups
- Division of Geological and Planetary Sciences