2025/09/10 by J. A. Hurowitz, Michael M. Tice, Abigail C. Allwood +86 · 4 voices · 72 citations
Engineering · Physics and Astronomy · #Astro and Planetary Science #Context (archaeology) #Mars Exploration Program #Martian #Martian surface #Meteorite #Mineral #Petrography #Planetary Science and Exploration #Pyrite #Sedimentary rock #Space Exploration and Technology
paper · pdf · doi:10.1038/s41586-025-09413-0
published in Nature 645(8080), 332-340 (Nature Portfolio)
openalex publication_date 2025/09/10 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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.