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SEDIMENTARY EVOLUTION OF THE JEZERO WESTERN FAN, MARS

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  • معلومة اضافية
    • Contributors:
      Department of Earth Science and Engineering Imperial College London; Imperial College London; Jet Propulsion Laboratory (JPL); NASA-California Institute of Technology (CALTECH); Laboratoire de Planétologie et Géosciences UMR_C 6112 (LPG); Le Mans Université (UM)-Université d'Angers (UA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST); Nantes Université - pôle Sciences et technologie; Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie; Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ); Institut de recherche en astrophysique et planétologie (IRAP); Université Toulouse III - Paul Sabatier (UT3); Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP); Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3); Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS); Planetary Science Institute Tucson (PSI); Department of Earth and Atmospheric Sciences Atlanta; Georgia Institute of Technology Atlanta; Department of Geological Sciences Gainesville (UF|Geological); University of Florida Gainesville (UF); Department of Earth, Planetary and Space Sciences Los Angeles (EPSS); University of California Los Angeles (UCLA); University of California (UC)-University of California (UC); Purdue University West Lafayette; Rice University Houston; Texas A&M University College Station; Stony Brook University SUNY (SBU); State University of New York (SUNY); Cornell University Ithaca (CU); Johns Hopkins University Applied Physics Laboratory Laurel, MD (APL); Department of Earth and Planetary Sciences Knoxville; The University of Tennessee Knoxville; Planetary Geosciences Institute Knoxville; The University of Tennessee Knoxville -The University of Tennessee Knoxville; Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE); École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL); Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS); School of Earth and Space Exploration Tempe (SESE); Arizona State University Tempe (ASU); Joanneum Research Forschungsgesellschaft mbH; Division of Geological and Planetary Sciences Pasadena; California Institute of Technology (CALTECH); Department of Earth, Atmospheric and Planetary Sciences MIT, Cambridge (EAPS); Massachusetts Institute of Technology (MIT); Institut de minéralogie, de physique des matériaux et de cosmochimie (IMPMC); Muséum national d'Histoire naturelle (MNHN)-Institut de recherche pour le développement IRD : UR206-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); University of Copenhagen = Københavns Universitet (UCPH); Berkeley Geochronology Center (BGC); NASA Johnson Space Center (JSC); NASA; Los Alamos National Laboratory (LANL); Lunar and Planetary Institute
    • بيانات النشر:
      HAL CCSD
    • الموضوع:
      2024
    • Collection:
      Le Mans Université: Archives Ouvertes (HAL)
    • الموضوع:
    • الموضوع:
      Pasadena (California), United States
    • نبذة مختصرة :
      International audience ; Sedimentary fans developed at the mouths of Martian valleys have been interpreted as the deposits of sustained surface water flow on early Mars building either fluvial fan systems or deltas into standing bodies of water [1]. Whilst much insight has been gleaned from orbital observations, it is only possible to constrain the character, relative timing and persistence of ancient aqueous activity on Mars through detailed on-the-ground interrogation of sedimentary successions built during fan growth. A prominent sedimentary fan deposit at the western margin of Jezero crater – the Western fan – has been interpreted from orbital data/observations to be a river delta that prograded into an ancient lake basin during the Late Noachian-Early Hesperian epochs on Mars (~3.6-3.8 Ga) [2]. The Western fan deposit forms a point-sourced depositional system developed at the mouth of Neretva Vallis, a valley system that is incised across the crater rim and has an extensive extra-crater catchment draining over diverse ancient geological units in Nili Planum [4]. The mechanism of crater rim breaching remains unconstrained. Between 2022 and 2023, the Mars 2020 Perseverance rover explored the Western fan, with the objective of characterizing its paleoenvironmental context and collecting a diverse suite of sedimentary rock samples for return to Earth via the Mars Sample Return mission. Perseverance has nowcompleted her traverse across the Western fan having commenced in the distal downstream sectors exposed at the erosional front of the fan and then crossing across its upper exposed surface toward the fan apex region near the mouth of Neretva Vallis. This transect provides a unique window into a Martian sediment routing system at a time when climate conditions permitted the flow of surface water. In this contribution, we review the overall sedimentary architecture of the fan and develop a model for its evolution based on detailed mapping of lithofacies changes across the fan. A first-order synoptic overview is ...
    • Relation:
      hal-04650004; https://hal.science/hal-04650004; https://hal.science/hal-04650004/document; https://hal.science/hal-04650004/file/3370.pdf
    • Rights:
      info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.12E1447C