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Geological, multispectral, and meteorological imaging results from the Mars 2020 Perseverance rover in Jezero crater.

James F BellJustin N MakiSanna AlwmarkBethany L EhlmannSarah A FagentsJohn P GrotzingerSanjeev GuptaAlexander G HayesKenneth E HerkenhoffBriony H N HorganJeffrey R JohnsonKjartan M KinchMark T LemmonMorten B MadsenJorge I NúñezGerhard PaarMelissa S RiceJames W RiceNicole SchmitzRobert J SullivanAlicia VaughanMichael J WolffAndreas BechtoldTanja BosakLouise E DuflotAlberto G FairénBrad GarczynskiRalf JaumannMarco MerusiChase MillionEleni RavanisDavid L ShusterJustin I SimonMichael St ClairChristian TateSebastian WalterBenjamin P WeissAlyssa M BaileyTanguy BertrandOlivier BeyssacAdrian J BrownPiluca Caballo-PeruchaMichael A CaplingerChristy M CaudillFrancesca CaryErnest CisnerosEdward A CloutisNathan CluffPaul CorliesKelsie CrawfordSabrina CurtisRobert DeenDarian DixonChristopher DonaldsonMegan BarringtonMichelle FichtStephanie FleronMichael HansenDavid HarkerRachel HowsonJoshua HuggettSamantha R JacobElsa H JensenOle B JensenMohini JodhpurkarJonathan JosephChristian JuarezLinda C KahOak KanineJessica KristensenTex KubackiKristiana LapoAngela MageeMichael MaimoneGreg L MehallLaura MehallJess MollerupDaniel Viudez-MoreirasKristen ParisKathryn E PowellFrank PreuskerJon ProtonCorrine RojasDanny SallurdayKim SaxtonEva L SchellerChristiana H SeegerMason StarrNathaniel T SteinNathalie TurenneJason K Van BeekAndrew G WinholdRachel Yingling
Published in: Science advances (2022)
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.
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