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      Diagenesis of the Clay‐Sulfate Stratigraphic Transition, Mount Sharp Group, Gale Crater, Mars

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          Abstract

          The diversity and abundance of diagenetic textures observed in sedimentary rocks of the clay‐sulfate transition recorded in the stratigraphic record of Gale crater are distinctive within the rover's traverse. This study catalogs all textures observed by the MAHLI instrument, including their abundances, morphologies, and cross‐cutting relationships in order to suggest a paragenetic sequence in which multiple episodes of diagenetic fluid flow were required to form co‐occurring color variations, pits, and nodules; secondary nodule populations; and two generations of Ca sulfate fracture‐filling vein precipitation. Spatial heterogeneities in the abundance and diversity of these textures throughout the studied stratigraphic section loosely correlate with stratigraphic unit, suggesting that grain size and compaction controls on fluid pathways influenced their formation; these patterns are especially prevalent in the Pontours member, where primary stratigraphy is entirely overprinted by a nodular fabric, and the base of the stratigraphic section, where increased textural diversity may be influenced by the underlying less permeable clay‐bearing rocks of the Glen Torridon region. Correlations between quantitative nodule abundance and subtle variations in measured bulk rock chemistry (especially MgO and SO 3 enrichment) by the Alpha Particle X‐Ray Spectrometer instrument suggest that an increase in Mg sulfate upsection is linked to precipitation of pore‐filling diagenetic cement. Due to a lack of sedimentological evidence for widespread evaporite or near‐surface crust formation of these Mg sulfates, we propose three alternative hypotheses for subsurface groundwater‐related remobilization of pre‐existing sulfates and reprecipitation at depth in pore spaces.

          Key Points

          • The clay‐sulfate transition region of Gale crater is marked by significant changes in diversity and abundance of diagenetic textures

          • Observed textures and their associated chemistry suggest several diagenetic episodes and concentrations of Mg sulfate in nodules and cement

          • We propose several groundwater‐based mechanisms to remobilize and precipitate Mg sulfate cement in the subsurface

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          Most cited references97

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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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            In situ evidence for an ancient aqueous environment at Meridiani Planum, Mars.

            Sedimentary rocks at Eagle crater in Meridiani Planum are composed of fine-grained siliciclastic materials derived from weathering of basaltic rocks, sulfate minerals (including magnesium sulfate and jarosite) that constitute several tens of percent of the rock by weight, and hematite. Cross-stratification observed in rock outcrops indicates eolian and aqueous transport. Diagenetic features include hematite-rich concretions and crystal-mold vugs. We interpret the rocks to be a mixture of chemical and siliciclastic sediments with a complex diagenetic history. The environmental conditions that they record include episodic inundation by shallow surface water, evaporation, and desiccation. The geologic record at Meridiani Planum suggests that conditions were suitable for biological activity for a period of time in martian history.
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              Deposition, exhumation, and paleoclimate of an ancient lake deposit, Gale crater, Mars

              The landforms of northern Gale crater on Mars expose thick sequences of sedimentary rocks. Based on images obtained by the Curiosity rover, we interpret these outcrops as evidence for past fluvial, deltaic, and lacustrine environments. Degradation of the crater wall and rim probably supplied these sediments, which advanced inward from the wall, infilling both the crater and an internal lake basin to a thickness of at least 75 meters. This intracrater lake system probably existed intermittently for thousands to millions of years, implying a relatively wet climate that supplied moisture to the crater rim and transported sediment via streams into the lake basin. The deposits in Gale crater were then exhumed, probably by wind-driven erosion, creating Aeolis Mons (Mount Sharp).
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                Author and article information

                Contributors
                cseeger@caltech.edu
                Journal
                J Geophys Res Planets
                J Geophys Res Planets
                10.1002/(ISSN)2169-9100
                JGRE
                Journal of Geophysical Research. Planets
                John Wiley and Sons Inc. (Hoboken )
                2169-9097
                2169-9100
                06 December 2024
                December 2024
                : 129
                : 12 ( doiID: 10.1002/jgre.v129.12 )
                : e2024JE008531
                Affiliations
                [ 1 ] Department of Geological and Planetary Sciences California Institute of Technology Pasadena CA USA
                Author notes
                [*] [* ] Correspondence to:

                C. H. Seeger,

                cseeger@ 123456caltech.edu

                Author information
                https://orcid.org/0000-0003-4993-9724
                Article
                JGRE22630 2024JE008531
                10.1029/2024JE008531
                11622355
                39649802
                aa704bd3-97ca-41f0-87ef-f88b5d7c3c1a
                © 2024 The Author(s).

                This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc/4.0/ License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes.

                History
                : 14 October 2024
                : 24 May 2024
                : 25 October 2024
                Page count
                Figures: 11, Tables: 0, Pages: 25, Words: 14604
                Funding
                Funded by: Jet Propulsion Laboratory , doi 10.13039/100006196;
                Categories
                Geochemistry
                Alteration and Weathering Processes
                Sedimentary Geochemistry
                Mineralogy and Petrology
                Alteration and Weathering Processes
                Planetary Sciences: Solar System Objects
                Mars
                Research Article
                Research Article
                Custom metadata
                2.0
                December 2024
                Converter:WILEY_ML3GV2_TO_JATSPMC version:6.5.1 mode:remove_FC converted:06.12.2024

                diagenesis,sedimentology,nodules,sulfate,curiosity,gale
                diagenesis, sedimentology, nodules, sulfate, curiosity, gale

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