Redox-driven mineral and organic associations in Jezero Crater, Mars
J. A. Hurowitz, Michael M. Tice, Abigail C. Allwood, Morgan L. Cable, K. P. Hand, Ashley Murphy, Kyle Uckert, J. F. Bell, Tanja Bosak, Adrian Broz, Elise Clavé, A. Cousin, Scott Davidoff, E. Dehouck, Kenneth A. Farley, Sanjeev Gupta, Svein‐Erik Hamran, Keyron Hickman‐Lewis, J. R. Johnson, Alexander Jones, Michael W. Jones, Peter S. Jørgensen, Linda C. Kah, H. Kalucha, T. V. Kizovski, David A. K. Pedersen, Yang Liu, F. M. McCubbin, E. L. Moreland, Gerhard Paar, D. A. Paige, A. C. Pascuzzo, M. S. Rice, M. E. Schmidt, K. L. Siebach, S. Siljeström, Justin I. Simon, K. M. Stack, A. Steele, Nicholas J. Tosca, A. H. Treiman, S. J. VanBommel, L. A. Wade, B. P. Weiss, R. C. Wiens, Kenneth H. Williford, Robert Barnes, P. Barr, Andreas Bechtold, Pierre Beck, Karim Benzerara, Sylvain Bernard, Olivier Beyssac, R. Bhartia, A. J. Brown, G. Caravaca, Emily Cardarelli, E. A. Cloutis, Alberto González Fairén, David Flannery, Teresa Fornaro, Thierry Fouchet, Bradley Garczynski, Felipe Gómez, Elisabeth M. Hausrath, Christopher M. Heirwegh, C. D. K. Herd, Joshua Huggett, John Leif Jørgensen, S. W. Lee, A. Y. Li, J. N. Maki, L. Mandon, N. Mangold, J. A. Manrique, Jesús Martínez‐Frías, Jorge I. Núñez, L. P. O’Neil, Brendan J. Orenstein, Nicole Phelan, Cathy Quantin‐Nataf, Patrick Russell, M. D. Schulte, Eva L. Scheller, Sunanda Sharma, David L. Shuster, A. Srivastava, Brittan Wogsland, U. Wolf
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 biosignatures1–7. 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. A geological, petrographic and geochemical survey of distinctive mudstone and conglomerate outcrops of the Bright Angel formation on Mars reveals textures, chemical and mineral characteristics, and organic signatures that warrant consideration as potential biosignatures.