Compositionally and density stratified igneous terrain in Jezero crater, Mars
Pyroxene
Lithology
DOI:
10.1126/sciadv.abo3399
Publication Date:
2022-08-25T17:58:10Z
AUTHORS (94)
ABSTRACT
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 revealed and intrusive terrain with compositional density stratification. The dominant lithology along traverse is basaltic, plagioclase enrichment stratigraphically higher locations. Stratigraphically lower, layered rocks are richer normative pyroxene. lowest observed unit has highest inferred olivine-rich coarse (1.5 millimeters) euhedral, relatively unweathered grains, suggesting cumulate This martian shows similarities meteorites, which also express olivine disequilibrium. Alteration materials including carbonates, sulfates, perchlorates, hydrated silicates, iron oxides pervasive but low abundance, brief lacustrine conditions. Orbital link broader Nili-Syrtis region, that density-driven stratification regional characteristic.
SUPPLEMENTAL MATERIAL
Coming soon ....
REFERENCES (79)
CITATIONS (93)
EXTERNAL LINKS
PlumX Metrics
RECOMMENDATIONS
FAIR ASSESSMENT
Coming soon ....
JUPYTER LAB
Coming soon ....