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dc.date.accessioned2026-04-28T21:10:30Z
dc.date.available2026-04-28T21:10:30Z
dc.date.issued2024-02-06
dc.identifier.urihttps://hdl.handle.net/1721.1/165732
dc.description.abstractThe Mars 2020 Perseverance rover has examined and sampled sulfate‐rich clastic rocks from the Hogwallow Flats member at Hawksbill Gap and the Yori Pass member at Cape Nukshak. Both strata are located on the Jezero crater western fan front, are lithologically and stratigraphically similar, and have been assigned to the Shenandoah formation. In situ analyses demonstrate that these are fine‐grained sandstones composed of phyllosilicates, hematite, Ca‐sulfates, Fe‐Mg‐sulfates, ferric sulfates, and possibly chloride salts. Sulfate minerals are found both as depositional grains and diagenetic features, including intergranular cement and vein‐ and vug‐cements. Here, we describe the possibility of various sulfate phases to preserve potential biosignatures and the record of paleoenvironmental conditions in fluid and solid inclusions, based on findings from analog sulfate‐rich rocks on Earth. The samples collected from these outcrops, Hazeltop and Bearwallow from Hogwallow Flats, and Kukaklek from Yori Pass, should be examined for such potential biosignatures and environmental indicators upon return to Earth.en_US
dc.language.isoen
dc.publisherAmerican Geophysical Unionen_US
dc.relation.isversionof10.1029/2023je008155en_US
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivativesen_US
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/en_US
dc.sourceAmerican Geophysical Unionen_US
dc.titleDepositional and Diagenetic Sulfates of Hogwallow Flats and Yori Pass, Jezero Crater: Evaluating Preservation Potential of Environmental Indicators and Possible Biosignatures From Past Martian Surface Waters and Groundwatersen_US
dc.typeArticleen_US
dc.identifier.citationBenison, K. C., Gill, K. K., Sharma, S., Siljeström, S., Zawaski, M., Bosak, T., et al. (2024). Depositional and diagenetic sulfates of Hogwallow Flats and Yori Pass, Jezero crater: Evaluating preservation potential of environmental indicators and possible biosignatures from past Martian surface waters and groundwaters. Journal of Geophysical Research: Planets, 129, e2023JE008155.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.relation.journalJournal of Geophysical Research: Planetsen_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.updated2026-04-28T21:04:23Z
dspace.orderedauthorsBenison, KC; Gill, KK; Sharma, S; Siljeström, S; Zawaski, M; Bosak, T; Broz, A; Clark, BC; Cloutis, E; Czaja, AD; Flannery, D; Fornaro, T; Gómez, F; Hand, K; Herd, CDK; Johnson, JR; Madariaga, JM; Madsen, MB; Martinez‐Frías, J; Nachon, M; Núñez, JI; Pedersen, DAK; Randazzo, N; Shuster, DL; Simon, J; Steele, A; Tate, C; Treiman, A; Uckert, K; Williams, AJ; Yanchilina, Aen_US
dspace.date.submission2026-04-28T21:04:25Z
mit.journal.volume129en_US
mit.journal.issue2en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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