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Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation.
Posiolova, L V; Lognonné, P; Banerdt, W B; Clinton, J; Collins, G S; Kawamura, T; Ceylan, S; Daubar, I J; Fernando, B; Froment, M; Giardini, D; Malin, M C; Miljkovic, K; Stähler, S C; Xu, Z; Banks, M E; Beucler, É; Cantor, B A; Charalambous, C; Dahmen, N; Davis, P; Drilleau, M; Dundas, C M; Durán, C; Euchner, F; Garcia, R F; Golombek, M; Horleston, A; Keegan, C; Khan, A; Kim, D; Larmat, C; Lorenz, R; Margerin, L; Menina, S; Panning, M; Pardo, C; Perrin, C; Pike, W T; Plasman, M; Rajsic, A; Rolland, L; Rougier, E; Speth, G; Spiga, A; Stott, A; Susko, D; Teanby, N A; Valeh, A; Werynski, A.
Afiliação
  • Posiolova LV; Malin Space Science Systems, San Diego, CA, USA.
  • Lognonné P; Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
  • Banerdt WB; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
  • Clinton J; Swiss Seismological Service, ETH Zurich, Zurich, Switzerland.
  • Collins GS; Department of Earth Science and Engineering, Imperial College London, London, UK.
  • Kawamura T; Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
  • Ceylan S; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Daubar IJ; Department of Earth, Environmental, and Planetary Sciences, Brown University, Providence, RI, USA.
  • Fernando B; Department of Earth Sciences, University of Oxford, Oxford, UK.
  • Froment M; Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
  • Giardini D; Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA.
  • Malin MC; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Miljkovic K; Malin Space Science Systems, San Diego, CA, USA.
  • Stähler SC; Space Science and Technology Centre, School of Earth and Planetary Sciences, Curtin University, Perth, WA, Australia.
  • Xu Z; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Banks ME; Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
  • Beucler É; NASA Goddard Space Flight Center, Greenbelt, MD, USA.
  • Cantor BA; Nantes Université, Université Angers, Le Mans Université, CNRS, UMR 6112, Laboratoire de Planétologie et Géosciences, Nantes, France.
  • Charalambous C; Malin Space Science Systems, San Diego, CA, USA.
  • Dahmen N; Department of Electrical and Electronic Engineering, Imperial College London, London, UK.
  • Davis P; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Drilleau M; Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA.
  • Dundas CM; Institut Supérieur de l'Aéronautique et de l'Espace ISAE-SUPAERO, Toulouse, France.
  • Durán C; U.S. Geological Survey, Astrogeology Science Center, Flagstaff, AZ, USA.
  • Euchner F; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Garcia RF; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Golombek M; Institut Supérieur de l'Aéronautique et de l'Espace ISAE-SUPAERO, Toulouse, France.
  • Horleston A; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
  • Keegan C; School of Earth Sciences, University of Bristol, Bristol, UK.
  • Khan A; Malin Space Science Systems, San Diego, CA, USA.
  • Kim D; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Larmat C; Physik-Institut, University of Zurich, Zurich, Switzerland.
  • Lorenz R; Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
  • Margerin L; Department of Geology, University of Maryland, College Park, MD, USA.
  • Menina S; Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA.
  • Panning M; Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA.
  • Pardo C; Institut de Recherche en Astrophysique et Planétologie, Université Toulouse III Paul Sabatier, CNRS, CNES, Toulouse, France.
  • Perrin C; Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
  • Pike WT; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
  • Plasman M; Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
  • Rajsic A; Nantes Université, Université Angers, Le Mans Université, CNRS, UMR 6112, Laboratoire de Planétologie et Géosciences, Nantes, France.
  • Rolland L; Department of Electrical and Electronic Engineering, Imperial College London, London, UK.
  • Rougier E; Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
  • Speth G; Space Science and Technology Centre, School of Earth and Planetary Sciences, Curtin University, Perth, WA, Australia.
  • Spiga A; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, IRD, Géoazur, Valbonne, France.
  • Stott A; Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA.
  • Susko D; Malin Space Science Systems, San Diego, CA, USA.
  • Teanby NA; Laboratoire de Météorologie Dynamique/IPSL, Sorbonne Université, CNRS, Ecole Normale Supérieure, PSL Research University, Ecole Polytechnique, Paris, France.
  • Valeh A; Institut Supérieur de l'Aéronautique et de l'Espace ISAE-SUPAERO, Toulouse, France.
  • Werynski A; Malin Space Science Systems, San Diego, CA, USA.
Science ; 378(6618): 412-417, 2022 10 28.
Article em En | MEDLINE | ID: mdl-36302013
Two >130-meter-diameter impact craters formed on Mars during the later half of 2021. These are the two largest fresh impact craters discovered by the Mars Reconnaissance Orbiter since operations started 16 years ago. The impacts created two of the largest seismic events (magnitudes greater than 4) recorded by InSight during its 3-year mission. The combination of orbital imagery and seismic ground motion enables the investigation of subsurface and atmospheric energy partitioning of the impact process on a planet with a thin atmosphere and the first direct test of martian deep-interior seismic models with known event distances. The impact at 35°N excavated blocks of water ice, which is the lowest latitude at which ice has been directly observed on Mars.
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2022 Tipo de documento: Article
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2022 Tipo de documento: Article