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      Evolution of a Lake Margin Recorded in the Sutton Island Member of the Murray Formation, Gale Crater, Mars

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          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.

          Plain Language Summary

          This study classifies sedimentary rock characteristics within an interval of sedimentary rock layers comprising the Sutton Island member, which is part of the Murray formation. The main goals of this study are to determine the ancient environments represented by the different sedimentary rock groups (facies) and to understand how ancient environments changed through time. Facies are grouped into two categories (associations) based on their distribution within the stratigraphy: Facies Association 1 (FA1) and Facies Association 2 (FA2). FA1 contains rocks with a range of sedimentary structures and grain sizes and formed via aqueous processes. The environment represented by FA1 is a delta plain adjacent to a lake. Facies Association 2 consists of one fine‐grained facies that represents deposition in a lake basin environment. The lowermost interval of stratigraphy is comprised of FA1 (delta plain), which transitions upward into the middle interval of stratigraphy comprised FA2 (lake) and subsequently returns to FA1 in the uppermost stratigraphic interval. Transitions between facies associations represent shifts in the ancient lake shoreline that may have been caused by lake‐level change. The delta plain and lake environments represented by FA1 and FA2 are consistent with facies in other members of the Murray formation.

          Key Points

          • The Sutton Island member consists of two distinct facies associations that record delta plain and lacustrine environments

          • The depositional history is indicative of a rapid transgression followed by forced regression

          • Facies record diverse aqueous processes and expand the range of environments interpreted in the Murray formation

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          Most cited references87

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          Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE)

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            A habitable fluvio-lacustrine environment at Yellowknife Bay, Gale crater, Mars.

            The Curiosity rover discovered fine-grained sedimentary rocks, which are inferred to represent an ancient lake and preserve evidence of an environment that would have been suited to support a martian biosphere founded on chemolithoautotrophy. This aqueous environment was characterized by neutral pH, low salinity, and variable redox states of both iron and sulfur species. Carbon, hydrogen, oxygen, sulfur, nitrogen, and phosphorus were measured directly as key biogenic elements; by inference, phosphorus is assumed to have been available. The environment probably had a minimum duration of hundreds to tens of thousands of years. These results highlight the biological viability of fluvial-lacustrine environments in the post-Noachian history of Mars.
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              Architectural-element analysis: A new method of facies analysis applied to fluvial deposits

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                Author and article information

                Contributors
                Journal
                Journal of Geophysical Research: Planets
                JGR Planets
                American Geophysical Union (AGU)
                2169-9097
                2169-9100
                January 2024
                January 11 2024
                January 2024
                : 129
                : 1
                Affiliations
                [1 ] Department of Earth and Planetary Sciences University of Tennessee, Knoxville Knoxville TN USA
                [2 ] Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA
                [3 ] Now at Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA
                [4 ] Division of Geological and Planetary Sciences California Institute of Technology Pasadena CA USA
                [5 ] Department of Earth Sciences and Engineering Imperial College London London UK
                [6 ] Department of Earth and Atmospheric Sciences Georgia Institute of Technology Atlanta GA USA
                [7 ] U.S. Geological Survey Astrogeology Science Center Flagstaff AZ USA
                [8 ] Department of Earth and Planetary Sciences Birkbeck, University of London London UK
                Article
                10.1029/2023JE007919
                fbe479c7-92e5-4c18-88ca-7d677673c0df
                © 2024

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