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      Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation

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      American Association for the Advancement of Science (AAAS)

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          Abstract

          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.

          An insightful impact

          On 24 December 2021, the seismometer for the InSight mission on Mars detected a large seismic event with a distinct signature. Posiolova et al . discovered that the event was caused by a meteor impact on the surface of Mars, which was confirmed by satellite observations of a newly formed 150-kilometer crater. The surface nature and size of the impact allowed Kim et al . to detect surface waves from the event, which have yet to be observed on Mars. These surface waves help to untangle the structure of the Martian crust, which has various amounts of volcanic and sedimentary rock, along with subsurface ice, in different regions of the planet (see the Perspective by Yang and Chen). The characteristics of the impact itself are important because they provide a seismic fingerprint of an impact event that is different from the marsquakes observed so far. —BG

          Abstract

          A new crater formed on the surface of Mars was detected with the seismometer on the InSight mission.

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          Most cited references66

          • Record: found
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          Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE)

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            • Abstract: not found
            • Article: not found

            Improved general circulation models of the Martian atmosphere from the surface to above 80 km

              Bookmark
              • Record: found
              • Abstract: not found
              • Article: not found

              Mars Global Surveyor Mars Orbiter Camera: Interplanetary cruise through primary mission

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                Journal
                Science
                Science
                American Association for the Advancement of Science (AAAS)
                0036-8075
                1095-9203
                October 28 2022
                October 28 2022
                : 378
                : 6618
                : 412-417
                Affiliations
                [1 ]Malin Space Science Systems, San Diego, CA, USA.
                [2 ]Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France.
                [3 ]Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
                [4 ]Swiss Seismological Service, ETH Zurich, Zurich, Switzerland.
                [5 ]Department of Earth Science and Engineering, Imperial College London, London, UK.
                [6 ]Institute of Geophysics, ETH Zurich, Zurich, Switzerland.
                [7 ]Department of Earth, Environmental, and Planetary Sciences, Brown University, Providence, RI, USA.
                [8 ]Department of Earth Sciences, University of Oxford, Oxford, UK.
                [9 ]Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA.
                [10 ]Space Science and Technology Centre, School of Earth and Planetary Sciences, Curtin University, Perth, WA, Australia.
                [11 ]NASA Goddard Space Flight Center, Greenbelt, MD, USA.
                [12 ]Nantes Université, Université Angers, Le Mans Université, CNRS, UMR 6112, Laboratoire de Planétologie et Géosciences, Nantes, France.
                [13 ]Department of Electrical and Electronic Engineering, Imperial College London, London, UK.
                [14 ]Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA.
                [15 ]Institut Supérieur de l’Aéronautique et de l’Espace ISAE-SUPAERO, Toulouse, France.
                [16 ]U.S. Geological Survey, Astrogeology Science Center, Flagstaff, AZ, USA.
                [17 ]School of Earth Sciences, University of Bristol, Bristol, UK.
                [18 ]Physik-Institut, University of Zurich, Zurich, Switzerland.
                [19 ]Department of Geology, University of Maryland, College Park, MD, USA.
                [20 ]Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA.
                [21 ]Institut de Recherche en Astrophysique et Planétologie, Université Toulouse III Paul Sabatier, CNRS, CNES, Toulouse, France.
                [22 ]Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, IRD, Géoazur, Valbonne, France.
                [23 ]Laboratoire de Météorologie Dynamique/IPSL, Sorbonne Université, CNRS, Ecole Normale Supérieure, PSL Research University, Ecole Polytechnique, Paris, France.
                Article
                10.1126/science.abq7704
                36302013
                f7fde69f-1e60-4b63-b58e-a4326f467c7d
                © 2022
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