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      The Curiosity Rover's Exploration of Glen Torridon, Gale Crater, Mars: An Overview of the Campaign and Scientific Results

      research-article
      1 , , 2 , 3 , 4 , 4 , 5 , 1 , 6 , 7 , 8 , 9 , 10 , 11 , 12 , 10 , 13 , 14 , 15 , 12 , 16 , 17 , 18 , 18 , 3 , 19 , 19 , 20 , 21 , 22 , 23 , 24 , 21 , 18 , 16 , 10 , 24
      Journal of Geophysical Research. Planets
      John Wiley and Sons Inc.

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          Abstract

          The Mars Science Laboratory rover, Curiosity, explored the clay mineral‐bearing Glen Torridon region for 1 Martian year between January 2019 and January 2021, including a short campaign onto the Greenheugh pediment. The Glen Torridon campaign sought to characterize the geology of the area, seek evidence of habitable environments, and document the onset of a potentially global climatic transition during the Hesperian era. Curiosity roved 5 km in total throughout Glen Torridon, from the Vera Rubin ridge to the northern margin of the Greenheugh pediment. Curiosity acquired samples from 11 drill holes during this campaign and conducted the first Martian thermochemolytic‐based organics detection experiment with the Sample Analysis at Mars instrument suite. The lowest elevations within Glen Torridon represent a continuation of lacustrine Murray formation deposits, but overlying widespread cross bedded sandstones indicate an interval of more energetic fluvial environments and prompted the definition of a new stratigraphic formation in the Mount Sharp group called the Carolyn Shoemaker formation. Glen Torridon hosts abundant phyllosilicates yet remains compositionally and mineralogically comparable to the rest of the Mount Sharp group. Glen Torridon samples have a great diversity and abundance of sulfur‐bearing organic molecules, which are consistent with the presence of ancient refractory organic matter. The Glen Torridon region experienced heterogeneous diagenesis, with the most striking alteration occurring just below the Siccar Point unconformity at the Greenheugh pediment. Results from the pediment campaign show that the capping sandstone formed within the Stimson Hesperian aeolian sand sea that experienced seasonal variations in wind direction.

          Key Points

          • Sedimentary facies within Glen Torridon record a transition from low‐energy lacustrine mudstones to higher‐energy fluvial sandstones

          • Glen Torridon hosts the highest clay mineral abundances observed thus far by Mars Science Laboratory (MSL) while remaining in family with the Mount Sharp group

          • Glen Torridon drill samples contain the greatest diversity of organic compounds yet detected by the MSL mission

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          Most cited references105

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          Global mineralogical and aqueous mars history derived from OMEGA/Mars Express data.

          Global mineralogical mapping of Mars by the Observatoire pour la Mineralogie, l'Eau, les Glaces et l'Activité (OMEGA) instrument on the European Space Agency's Mars Express spacecraft provides new information on Mars' geological and climatic history. Phyllosilicates formed by aqueous alteration very early in the planet's history (the "phyllocian" era) are found in the oldest terrains; sulfates were formed in a second era (the "theiikian" era) in an acidic environment. Beginning about 3.5 billion years ago, the last era (the "siderikian") is dominated by the formation of anhydrous ferric oxides in a slow superficial weathering, without liquid water playing a major role across the planet.
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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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                Author and article information

                Contributors
                kbennett@usgs.gov
                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
                30 December 2022
                January 2023
                : 128
                : 1 ( doiID: 10.1002/jgre.v128.1 )
                : e2022JE007185
                Affiliations
                [ 1 ] Astrogeology Science Center U.S. Geological Survey Flagstaff AZ USA
                [ 2 ] Department of Earth and Environmental Sciences University of Minnesota Minneapolis MN USA
                [ 3 ] Division of Geologic and Planetary Sciences California Institute of Technology Pasadena CA USA
                [ 4 ] Department of Earth and Planetary Science University of California, Berkeley Berkeley CA USA
                [ 5 ] Department of Earth and Planetary Sciences University of Tennessee Knoxville TN USA
                [ 6 ] Texas State University JETS NASA Johnson Space Center Houston TX USA
                [ 7 ] Department of Geological Sciences University of Florida Gainesville FL USA
                [ 8 ] Department of Geosciences The Pennsylvania State University University Park PA USA
                [ 9 ] Université de Lyon UCBL ENSL UJM CNRS LGL‐TPE Villeurbanne France
                [ 10 ] NASA Goddard Space Flight Center Greenbelt MD USA
                [ 11 ] Jacobs Technology Houston TX USA
                [ 12 ] NASA Johnson Space Center Houston TX USA
                [ 13 ] Department of Biology Georgetown University Washington DC USA
                [ 14 ] Laboratoire Atmosphère, Observations Spatiales (LATMOS), LATMOS/IPSL UVSQ Université Paris‐Saclay, Sorbonne Université, CNRS Guyancourt France
                [ 15 ] Department of Earth Sciences and Engineering Imperial College London London UK
                [ 16 ] Lunar and Planetary Institute Houston TX USA
                [ 17 ] NASA Ames Research Center Moffett Field CA USA
                [ 18 ] Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA
                [ 19 ] Planetary and Space Science Centre University of New Brunswick Fredericton NB Canada
                [ 20 ] Los Alamos National Laboratory Los Alamos NM USA
                [ 21 ] Earth Atmosphere and Planetary Science Purdue University West Lafayette IN USA
                [ 22 ] CCAPS Cornell University Ithaca NY USA
                [ 23 ] Department of Earth and Planetary Sciences Washington University in St. Louis St. Louis MO USA
                [ 24 ] IRAP Université de Toulouse CNRS CNES Toulouse France
                Author notes
                [*] [* ] Correspondence to:

                K. A. Bennett,

                kbennett@ 123456usgs.gov

                Author information
                https://orcid.org/0000-0001-8105-7129
                https://orcid.org/0000-0002-2013-7456
                https://orcid.org/0000-0002-2626-1132
                https://orcid.org/0000-0001-7512-7813
                https://orcid.org/0000-0002-1235-9016
                https://orcid.org/0000-0003-0136-6373
                https://orcid.org/0000-0002-1368-4494
                https://orcid.org/0000-0001-9120-2991
                https://orcid.org/0000-0002-3036-170X
                https://orcid.org/0000-0002-8887-4313
                https://orcid.org/0000-0003-1206-1639
                https://orcid.org/0000-0002-0783-1064
                https://orcid.org/0000-0001-6725-0555
                https://orcid.org/0000-0003-4017-5158
                https://orcid.org/0000-0003-2665-286X
                https://orcid.org/0000-0001-9324-1257
                https://orcid.org/0000-0002-5444-952X
                https://orcid.org/0000-0003-4561-3663
                https://orcid.org/0000-0003-0895-1153
                https://orcid.org/0000-0003-2911-9032
                https://orcid.org/0000-0003-4191-598X
                https://orcid.org/0000-0002-2854-0362
                https://orcid.org/0000-0001-7823-7794
                https://orcid.org/0000-0001-6314-9724
                https://orcid.org/0000-0002-8073-2839
                https://orcid.org/0000-0003-3089-1986
                https://orcid.org/0000-0002-4138-0471
                Article
                JGRE21942 2022JE007185
                10.1029/2022JE007185
                10078523
                dbd9ec6e-891b-4b9c-8456-adb2ba7f57a9
                © 2022 The Authors. California Institute of Technology. Government sponsorship acknowledged. This article has been contributed to by U.S. Government employees and their work is in the public domain in the USA.

                This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc-nd/4.0/ License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.

                History
                : 10 May 2022
                : 18 January 2022
                : 12 May 2022
                Page count
                Figures: 24, Tables: 2, Pages: 31, Words: 19581
                Funding
                Funded by: MSL
                Funded by: National Aeronautics and Space Administration
                Award ID: 80NM0018D0004
                Categories
                The Curiosity rover's investigation of Glen Torridon and the surrounding area
                Atmospheric Composition and Structure
                Planetary Atmospheres
                Geochemistry
                Planetary Geochemistry
                Mineralogy and Petrology
                Planetary Mineralogy and Petrology
                Planetary Sciences: Astrobiology
                Planetary Atmospheres, Clouds, and Hazes
                Planetary Sciences: Solid Surface Planets
                Composition
                Erosion and Weathering
                Hydrology and Fluvial Processes
                Surface Materials and Properties
                Planetary Sciences: Solid Surface Planets
                Atmospheres
                Planetary Sciences: Fluid Planets
                Atmospheres
                Composition
                Planetary Sciences: Comets and Small Bodies
                Atmospheres
                Composition
                Planetary Sciences: Solar System Objects
                Mars
                Research Article
                Research Article
                Custom metadata
                2.0
                January 2023
                Converter:WILEY_ML3GV2_TO_JATSPMC version:6.2.7 mode:remove_FC converted:06.04.2023

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