CRISM Detections of Hydrated Silica in Mt Sharp, Gale Crater

dc.contributor.authorFox, V. K.
dc.contributor.authorDundar, M. M.
dc.contributor.authorEhlmann, B. L.
dc.contributor.departmentComputer and Information Science, School of Scienceen_US
dc.date.accessioned2021-09-24T20:50:51Z
dc.date.available2021-09-24T20:50:51Z
dc.date.issued2020-03
dc.description.abstractMachine learning-enabled detections of hydrated silica in the Mt Sharp stratigraphic succession place constraints on alteration pathways in Gale Crater.en_US
dc.eprint.versionAuthor's manuscripten_US
dc.identifier.citationFox, V. K., Dundar, M. M., & Ehlmann, B. L. (2020). CRISM Detections of Hydrated Silica in Mt Sharp, Gale Crater. 51st Lunar and Planetary Science Conference, held 16-20 March, 2020 at The Woodlands, Texas. LPI Contribution No. 2326.en_US
dc.identifier.urihttps://hdl.handle.net/1805/26647
dc.language.isoenen_US
dc.publisherNASAen_US
dc.relation.journal51st Lunar and Planetary Science Conferenceen_US
dc.rightsPublisher Policyen_US
dc.sourceAuthoren_US
dc.subjectCompact Reconnaissance Imaging Spectrometer for Mars (CRISM)en_US
dc.subjecthydrated silicaen_US
dc.subjectGale Crateren_US
dc.titleCRISM Detections of Hydrated Silica in Mt Sharp, Gale Crateren_US
dc.typeConference proceedingsen_US
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