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dc.contributor.authorPosiolova, L.V.
dc.contributor.authorLognonné, P.
dc.contributor.authorBanerdt, W.B.
dc.contributor.authorClinton, J.
dc.contributor.authorCollins, G.S.
dc.contributor.authorKawamura, T.
dc.contributor.authorCeylan, S.
dc.contributor.authorDaubar, I.J.
dc.contributor.authorFernando, B.
dc.contributor.authorFroment, M.
dc.contributor.authorGiardini, D.
dc.contributor.authorMalin, M.C.
dc.contributor.authorMiljković, Katarina
dc.contributor.authorStähler, S.C.
dc.contributor.authorXu, Z.
dc.contributor.authorBanks, M.E.
dc.contributor.authorBeucler
dc.contributor.authorCantor, B.A.
dc.contributor.authorCharalambous, C.
dc.contributor.authorDahmen, N.
dc.contributor.authorDavis, P.
dc.contributor.authorDrilleau, M.
dc.contributor.authorDundas, C.M.
dc.contributor.authorDurán, C.
dc.contributor.authorEuchner, F.
dc.contributor.authorGarcia, R.F.
dc.contributor.authorGolombek, M.
dc.contributor.authorHorleston, A.
dc.contributor.authorKeegan, C.
dc.contributor.authorKhan, A.
dc.contributor.authorKim, D.
dc.contributor.authorLarmat, C.
dc.contributor.authorLorenz, R.
dc.contributor.authorMargerin, L.
dc.contributor.authorMenina, S.
dc.contributor.authorPanning, M.
dc.contributor.authorPardo, C.
dc.contributor.authorPerrin, C.
dc.contributor.authorPike, W.T.
dc.contributor.authorPlasman, M.
dc.contributor.authorRajšić, Andrea
dc.contributor.authorRolland, L.
dc.contributor.authorRougier, E.
dc.contributor.authorSpeth, G.
dc.contributor.authorSpiga, A.
dc.contributor.authorStott, A.
dc.contributor.authorSusko, D.
dc.contributor.authorTeanby, N.A.
dc.contributor.authorValeh, A.
dc.contributor.authorWerynski, A.
dc.contributor.authorWójcicka, N.
dc.contributor.authorZenhäusern, G.
dc.date.accessioned2023-01-28T02:01:14Z
dc.date.available2023-01-28T02:01:14Z
dc.date.issued2022
dc.identifier.citationPosiolova, L.V. and Lognonné, P. and Banerdt, W.B. and Clinton, J. and Collins, G.S. and Kawamura, T. and Ceylan, S. et al. 2022. Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation. Science. 378 (6618): pp. 412-417.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/90182
dc.identifier.doi10.1126/science.abq7704
dc.description.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.

dc.languageEnglish
dc.publisherAMER ASSOC ADVANCEMENT SCIENCE
dc.relation.sponsoredbyhttp://purl.org/au-research/grants/arc/DP180100661
dc.relation.sponsoredbyhttp://purl.org/au-research/grants/arc/FT210100063
dc.subjectScience & Technology
dc.subjectMultidisciplinary Sciences
dc.subjectScience & Technology - Other Topics
dc.subjectWAVES
dc.subjectEXCITATION
dc.subjectEARTH
dc.titleLargest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation
dc.typeJournal Article
dcterms.source.volume378
dcterms.source.number6618
dcterms.source.startPage412
dcterms.source.endPage417
dcterms.source.issn0036-8075
dcterms.source.titleScience
dc.date.updated2023-01-28T02:01:14Z
curtin.accessStatusFulltext not available
curtin.contributor.orcidMiljković, Katarina [0000-0001-8644-8903]
curtin.contributor.researcheridMiljković, Katarina [D-4844-2013]
dcterms.source.eissn1095-9203
curtin.contributor.scopusauthoridMiljković, Katarina [35219281700]


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