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IN SITU INVESTIGATION OF THE GEDIZ VALLIS RIDGE: A REMNANT LATE-STAGE DEBRIS FLOW DOMINATED FAN DEPOSIT IN GALE CRATER

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  • معلومة اضافية
    • Contributors:
      Department of Earth and Planetary Science UC Berkeley (EPS); University of California Berkeley (UC Berkeley); University of California (UC)-University of California (UC); Department of Earth and Planetary Sciences Knoxville; The University of Tennessee Knoxville; 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); Department of Earth Science and Engineering Imperial College London; Imperial College London; Division of Geological and Planetary Sciences Pasadena; California Institute of Technology (CALTECH); Smithsonian Institution; Department of Earth, Atmospheric, and Planetary Sciences, Purdue University; Purdue University West Lafayette; Jet Propulsion Laboratory (JPL); NASA-California Institute of Technology (CALTECH); Department of Earth and Planetary Sciences St Louis; Washington University in Saint Louis (WUSTL); 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); Carleton College; United States Geological Survey, Astrogeology Science Center (USGS), Flagstaff, United States (USGS); Planetary Science Institute Tucson (PSI); Johns Hopkins University (JHU); University of California Santa Cruz (UC Santa Cruz); University of California (UC); University of Chicago; Lunar and Planetary Institute
    • بيانات النشر:
      HAL CCSD
    • الموضوع:
      2024
    • Collection:
      Météo-France: HAL
    • الموضوع:
    • نبذة مختصرة :
      International audience ; Numerous studies using orbital HiRISE and CTX data show evidence for extensive fan formation across the Martian surface [1, 2]. Fan-shaped deposits record a combination of fluvial, debris flow, and deltaic processes, with many fans likely forming during the late Hesperian or Amazonian [1, 3]. Curiosity-based observations of the deeply eroded deposits of the Gediz Vallis ridge (GVR), near the base of Aeolis Mons (Mt. Sharp), provide our first cross-sectional observation of a Martian fan, revealing episodic deposition by debris flows and reworking by fluvial processes.
    • Relation:
      hal-04442711; https://hal.science/hal-04442711; https://hal.science/hal-04442711/document; https://hal.science/hal-04442711/file/1770.pdf
    • Rights:
      info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.A11A990C