Sie befinden Sich nicht im Netzwerk der Universität Paderborn. Der Zugriff auf elektronische Ressourcen ist gegebenenfalls nur via VPN oder Shibboleth (DFN-AAI) möglich. mehr Informationen...
Science advances, 2022-08, Vol.8 (34), p.eabo3399-eabo3399
2022

Details

Autor(en) / Beteiligte
Titel
Compositionally and density stratified igneous terrain in Jezero crater, Mars
Ist Teil von
  • Science advances, 2022-08, Vol.8 (34), p.eabo3399-eabo3399
Ort / Verlag
United States: American Association for the Advancement of Science (AAAS)
Erscheinungsjahr
2022
Link zum Volltext
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
  • Before Perseverance, Jezero crater's floor was variably hypothesized to have a lacustrine, lava, volcanic airfall, or aeolian origin. SuperCam observations in the first 286 Mars days on Mars revealed a volcanic and intrusive terrain with compositional and density stratification. The dominant lithology along the traverse is basaltic, with plagioclase enrichment in stratigraphically higher locations. Stratigraphically lower, layered rocks are richer in normative pyroxene. The lowest observed unit has the highest inferred density and is olivine-rich with coarse (1.5 millimeters) euhedral, relatively unweathered grains, suggesting a cumulate origin. This is the first martian cumulate and shows similarities to martian meteorites, which also express olivine disequilibrium. Alteration materials including carbonates, sulfates, perchlorates, hydrated silicates, and iron oxides are pervasive but low in abundance, suggesting relatively brief lacustrine conditions. Orbital observations link the Jezero floor lithology to the broader Nili-Syrtis region, suggesting that density-driven compositional stratification is a regional characteristic.
Sprache
Englisch
Identifikatoren
ISSN: 2375-2548
eISSN: 2375-2548
DOI: 10.1126/sciadv.abo3399
Titel-ID: cdi_swepub_primary_oai_DiVA_org_ri_60082

Weiterführende Literatur

Empfehlungen zum selben Thema automatisch vorgeschlagen von bX