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The rock abrasion record at Gale Crater: Mars Science Laboratory results from Bradbury Landing to Rocknest

Authors :
Fred Calef
R. A. Yingst
Nina Lanza
Yves Langevin
K. E. Herkenhoff
P. Y. Meslin
Roger C. Wiens
Diana L. Blaney
Sylvestre Maurice
Nilton O. Renno
Claire E. Newman
M. E. Richardson
Melissa S. Rice
M. A. de Pablo
Bernard Hallet
Violaine Sautter
Nathan T. Bridges
Gary Kocurek
R. S. Sletten
N. Mangold
Patrick Pinet
S. Le Mouélic
Kevin W. Lewis
Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL)
Jet Propulsion Laboratory (JPL)
NASA-California Institute of Technology (CALTECH)
Department of Earth and Space Sciences [Seattle]
University of Washington [Seattle]
United States Geological Survey [Reston] (USGS)
Los Alamos National Laboratory (LANL)
Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG)
Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST)
Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Ashima Research
Universidad de Alcalá - University of Alcalá (UAH)
Department of Geological Sciences [Austin]
Jackson School of Geosciences (JSG)
University of Texas at Austin [Austin]-University of Texas at Austin [Austin]
Institute d’Astrophysique Spatiale
Université Paris-Sud
Department of Geosciences [Princeton]
Princeton University
Institut de recherche en astrophysique et planétologie (IRAP)
Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP)
Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)
Department of Earth and Atmospheric Sciences [Michigan]
Central Michigan University (CMU)
Division of Geological and Planetary Sciences [Pasadena]
California Institute of Technology (CALTECH)
Lab Mineral and Cosmochim Museum
Planetary Science Institute [Tucson] (PSI)
Institut d'astrophysique spatiale (IAS)
Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)
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)
Source :
Journal of Geophysical Research. Planets, Journal of Geophysical Research. Planets, Wiley-Blackwell, 2014, 119 (6), pp.1374-1389. ⟨10.1002/2013JE004579⟩, Journal of Geophysical Research. Planets, 2014, 119 (6), pp.1374-1389. ⟨10.1002/2013JE004579⟩
Publication Year :
2014
Publisher :
HAL CCSD, 2014.

Abstract

International audience; Ventifacts, rocks abraded by wind-borne particles, are found in Gale Crater, Mars. In the eastwarddrive from “Bradbury Landing” to “Rocknest,” they account for about half of the float and outcrop seen byCuriosity’s cameras. Many are faceted and exhibit abrasion textures found at a range of scales, fromsubmillimeter lineations to centimeter-scale facets, scallops, flutes, and grooves. The drive path geometryin the first 100 sols of the mission emphasized the identification of abrasion facets and textures formedby westerly flow. This upwind direction is inconsistent with predictions based on models and the orientationof regional dunes, suggesting that these ventifact features formed from very rare high-speed winds. Theabsence of active sand and evidence for deflation in the area indicates that most of the ventifacts are fossilfeatures experiencing little abrasion today.

Details

Language :
English
ISSN :
21699097 and 21699100
Database :
OpenAIRE
Journal :
Journal of Geophysical Research. Planets, Journal of Geophysical Research. Planets, Wiley-Blackwell, 2014, 119 (6), pp.1374-1389. ⟨10.1002/2013JE004579⟩, Journal of Geophysical Research. Planets, 2014, 119 (6), pp.1374-1389. ⟨10.1002/2013JE004579⟩
Accession number :
edsair.doi.dedup.....70a1c58cd59d1810fc54f2952cc09cf2
Full Text :
https://doi.org/10.1002/2013JE004579⟩