Diverse Lava Flow Morphologies in the Stratigraphy of the Jezero Crater Floor

Research output: Contribution to journalJournal articleResearchpeer-review


  • Fulltext

    Final published version, 4.81 MB, PDF document

  • S. Alwmark
  • B. Horgan
  • A. Udry
  • A. Bechtold
  • S. Fagents
  • E. Ravanis
  • L. Crumpler
  • N. Schmitz
  • E. Cloutis
  • A. Brown
  • D. Flannery
  • O. Gasnault
  • J. Grotzinger
  • S. Gupta
  • L. Kah
  • P. Kelemen
  • Kinch, Kjartan Münster
  • J. Núñez

We present a combined geomorphologic, multispectral, and geochemical analysis of crater floor rocks in Jezero crater based on data obtained by the Mast Camera Zoom and SuperCam instruments onboard the NASA Mars 2020 Perseverance rover. The combined data from this analysis together with the results of a comparative study with geologic sites on Earth allows us to interpret the origins of rocks exposed along the Artuby ridge, a ∼900 m long scarp of lower Máaz formation rocks. The ridge exposes rocks belonging to two morphologically distinct members, Artuby and Rochette, both of which have basaltic composition and are spectrally indistinguishable in our analysis. Artuby rocks consist of morphologically distinct units that alternate over the ridge, bulbous, hummocky, layers with varying thicknesses that in places appear to have flowed over underlying strata, and sub-planar thinner laterally continuous layers with variable friability. The Rochette member has a massive appearance with pronounced pitting and sub-horizontal partings. Our findings are most consistent with a primary igneous emplacement as lava flows, through multiple eruptions, and we propose that the thin layers result either from preferential weathering, interbedded ash/tephra layers, ʻaʻā clinker layers, or aeolian deposition. Our analyses provide essential geologic context for the Máaz formation samples that will be returned to Earth and highlight the diversity and complexity of geologic processes on Mars not visible from orbit.

Original languageEnglish
Article numbere2022JE007446
JournalJournal of Geophysical Research - Planets
Issue number7
Number of pages24
Publication statusPublished - 2023

Bibliographical note

Publisher Copyright:
© 2023. The Authors.

    Research areas

  • Artuby, Jezero crater, Lava, Maaz formation, Mars 2020 Perseverance

ID: 361385436