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Redox-driven mineral and organic associations in Jezero Crater, Mars

  • Joel A. Hurowitz
  • , M. M. Tice
  • , A. C. Allwood
  • , M. L. Cable
  • , K. P. Hand
  • , A. E. Murphy
  • , K. Uckert
  • , J. F. Bell
  • , T. Bosak
  • , A. P. Broz
  • , E. Clavé
  • , A. Cousin
  • , S. Davidoff
  • , E. Dehouck
  • , K. A. Farley
  • , S. Gupta
  • , S. E. Hamran
  • , K. Hickman-Lewis
  • , J. R. Johnson
  • , A. J. Jones
  • M. W.M. Jones, P. S. Jørgensen, L. C. Kah, H. Kalucha, T. V. Kizovski, D. A. Klevang, Y. Liu, F. M. McCubbin, E. L. Moreland, G. Paar, D. A. Paige, A. C. Pascuzzo, M. S. Rice, M. E. Schmidt, K. L. Siebach, S. Siljeström, J. I. Simon, K. M. Stack, A. Steele, N. J. Tosca, A. H. Treiman, S. J. VanBommel, L. A. Wade, B. P. Weiss, R. C. Wiens, K. H. Williford, R. Barnes, P. A. Barr, A. Bechtold, P. Beck, K. Benzerara, S. Bernard, O. Beyssac, R. Bhartia, A. J. Brown, G. Caravaca, E. L. Cardarelli, E. A. Cloutis, A. G. Fairén, D. T. Flannery, T. Fornaro, T. Fouchet, B. Garczynski, F. Goméz, E. M. Hausrath, C. M. Heirwegh, C. D.K. Herd, J. E. Huggett, J. L. Jørgensen, S. W. Lee, A. Y. Li, J. N. Maki, L. Mandon, N. Mangold, J. A. Manrique, J. Martínez-Frías, J. I. Núñez, L. P. O’Neil, B. J. Orenstein, N. Phelan, C. Quantin-Nataf, P. Russell, M. D. Schulte, E. Scheller, S. Sharma, D. L. Shuster, A. Srivastava, B. V. Wogsland, Z. U. Wolf
  • Texas A&M University
  • California Institute of Technology
  • Planetary Science Institute
  • Arizona State University
  • Massachusetts Institute of Technology
  • Purdue University
  • German Aerospace Center
  • Institute de Recherche en Astrophysique et Planétologie
  • Université Lyon
  • Imperial College London
  • University of Oslo
  • Birkbeck University of London
  • Johns Hopkins University Applied Physics Laboratory
  • Queensland University of Technology
  • Technical University of Denmark
  • University of Tennessee
  • Brock University
  • NASA Johnson Space Center
  • Rice University
  • Joanneum Research
  • University of California at Los Angeles
  • Malin Space Science Systems
  • Western Washington University
  • RISE Research Institutes of Sweden
  • Carnegie Science Earth and Planets Laboratory
  • University of Cambridge
  • Universities Space Research Association
  • Washington University St. Louis
  • Blue Marble Space Institute of Science
  • University of Vienna
  • Université de Grenoble Alpes, ISTerre
  • Physique des Milieux Condensés (CNRS URA 782) Universiteé P et M Curie
  • Sorbonne Université
  • Photon Systems Inc.
  • Plancius Research
  • University Paul Sabatier
  • University of Winnipeg
  • Centro de Astrobiología (INTA-CSIC)
  • Osservatorio Astrofisico Di Arcetri, Florence
  • PSL University
  • University of Nevada, Las Vegas
  • University of Alberta
  • University of Washington
  • UJF Grenoble 1 CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), UMR 5274
  • Nantes Université
  • University of Valladolid
  • CSIC-UCM - Instituto de Geociencias (IGEO)
  • National Aeronautics and Space Administration
  • University of California at Berkeley
  • Los Alamos National Laboratory

Research output: Contribution to journalArticlepeer-review

53 Scopus citations

Abstract

The Perseverance rover has explored and sampled igneous and sedimentary rocks within Jezero Crater to characterize early Martian geological processes and habitability and search for potential biosignatures1, 2, 3, 4, 5, 6–7. Upon entering Neretva Vallis, on Jezero Crater’s western edge8, Perseverance investigated distinctive mudstone and conglomerate outcrops of the Bright Angel formation. Here we report a detailed geological, petrographic and geochemical survey of these rocks and show that organic-carbon-bearing mudstones in the Bright Angel formation contain submillimetre-scale nodules and millimetre-scale reaction fronts enriched in ferrous iron phosphate and sulfide minerals, likely vivianite and greigite, respectively. This organic carbon appears to have participated in post-depositional redox reactions that produced the observed iron-phosphate and iron-sulfide minerals. Geological context and petrography indicate that these reactions occurred at low temperatures. Within this context, we review the various pathways by which redox reactions that involve organic matter can produce the observed suite of iron-, sulfur- and phosphorus-bearing minerals in laboratory and natural environments on Earth. Ultimately, we conclude that analysis of the core sample collected from this unit using high-sensitivity instrumentation on Earth will enable the measurements required to determine the origin of the minerals, organics and textures it contains.

Original languageEnglish
Pages (from-to)332-340
Number of pages9
JournalNature
Volume645
Issue number8080
DOIs
StatePublished - Sep 11 2025

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