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dc.date.accessioned2023-02-09T19:52:36Z
dc.date.available2023-02-09T19:52:36Z
dc.date.issued2022-11-25
dc.identifier.urihttps://hdl.handle.net/1721.1/147991
dc.description.abstract<jats:p>Perseverance’s Mastcam-Z instrument provides high-resolution stereo and multispectral images with a unique combination of spatial resolution, spatial coverage, and wavelength coverage along the rover’s traverse in Jezero crater, Mars. Images reveal rocks consistent with an igneous (including volcanic and/or volcaniclastic) and/or impactite origin and limited aqueous alteration, including polygonally fractured rocks with weathered coatings; massive boulder-forming bedrock consisting of mafic silicates, ferric oxides, and/or iron-bearing alteration minerals; and coarsely layered outcrops dominated by olivine. Pyroxene dominates the iron-bearing mineralogy in the fine-grained regolith, while olivine dominates the coarse-grained regolith. Solar and atmospheric imaging observations show significant intra- and intersol variations in dust optical depth and water ice clouds, as well as unique examples of boundary layer vortex action from both natural (dust devil) and Ingenuity helicopter–induced dust lifting. High-resolution stereo imaging also provides geologic context for rover operations, other instrument observations, and sample selection, characterization, and confirmation.</jats:p>en_US
dc.language.isoen
dc.publisherAmerican Association for the Advancement of Science (AAAS)en_US
dc.relation.isversionof10.1126/sciadv.abo4856en_US
dc.rightsCreative Commons Attribution NonCommercial License 4.0en_US
dc.rights.urihttps://creativecommons.org/licenses/by-nc/4.0/en_US
dc.sourceScience Advancesen_US
dc.titleGeological, multispectral, and meteorological imaging results from the Mars 2020 Perseverance rover in Jezero crateren_US
dc.typeArticleen_US
dc.identifier.citation2022. "Geological, multispectral, and meteorological imaging results from the Mars 2020 Perseverance rover in Jezero crater." Science Advances, 8 (47).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.relation.journalScience Advancesen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2023-02-09T19:40:36Z
dspace.orderedauthorsBell, JF; Maki, JN; Alwmark, S; Ehlmann, BL; Fagents, SA; Grotzinger, JP; Gupta, S; Hayes, A; Herkenhoff, KE; Horgan, BHN; Johnson, JR; Kinch, KB; Lemmon, MT; Madsen, MB; Núñez, JI; Paar, G; Rice, M; Rice, JW; Schmitz, N; Sullivan, R; Vaughan, A; Wolff, MJ; Bechtold, A; Bosak, T; Duflot, LE; Fairén, AG; Garczynski, B; Jaumann, R; Merusi, M; Million, C; Ravanis, E; Shuster, DL; Simon, J; St. Clair, M; Tate, C; Walter, S; Weiss, B; Bailey, AM; Bertrand, T; Beyssac, O; Brown, AJ; Caballo-Perucha, P; Caplinger, MA; Caudill, CM; Cary, F; Cisneros, E; Cloutis, EA; Cluff, N; Corlies, P; Crawford, K; Curtis, S; Deen, R; Dixon, D; Donaldson, C; Barrington, M; Ficht, M; Fleron, S; Hansen, M; Harker, D; Howson, R; Huggett, J; Jacob, S; Jensen, E; Jensen, OB; Jodhpurkar, M; Joseph, J; Juarez, C; Kah, LC; Kanine, O; Kristensen, J; Kubacki, T; Lapo, K; Magee, A; Maimone, M; Mehall, GL; Mehall, L; Mollerup, J; Viúdez-Moreiras, D; Paris, K; Powell, KE; Preusker, F; Proton, J; Rojas, C; Sallurday, D; Saxton, K; Scheller, E; Seeger, CH; Starr, M; Stein, N; Turenne, N; Van Beek, J; Winhold, AG; Yingling, Ren_US
dspace.date.submission2023-02-09T19:40:39Z
mit.journal.volume8en_US
mit.journal.issue47en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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