Fe-phosphates in Jezero Crater as evidence for an ancient habitable environment on Mars

Phosphorus is an essential component for life, and in-situ identification of phosphate minerals that formed in aqueous conditions directly contributes toward one of the main goals of the Mars 2020 Perseverance rover: to seek signs of ancient habitable environments. In Jezero crater, proximity science analyses within a conglomerate outcrop, "Onahu" demonstrate the presence of rare Fe<sup>3+</sup>-bearing phosphate minerals (likely metavivianite, ferrolaueite, (ferro)beraunite, and/or santabarbaraite) embedded in a carbonate-rich matrix. While Fe-phosphates have been inferred previously on Mars, this work presents the most definitive in-situ identification of martian Fe-phosphate minerals to date, using textural, chemical, spectral, and diffraction analyses of discrete green-blue grains. The Fe-phosphate minerals' textural context along with comparisons to Earth analogs suggest they likely formed after oxidation of Fe<sup>2+</sup>-phosphate vivianite, the most common Fe-phosphate in sedimentary environments on Earth, often associated with microbial activity and organics. While there is no obvious evidence of biological inputs in Onahu, if the Fe-phosphates' formation environment was similar to vivianite-rich sedimentary environments on Earth, these minerals likely originally precipitated in conditions favorable to potential martian life - in a low temperature, reducing aqueous medium with high concentrations of bio-limiting elements, and Fe-redox gradients that could provide an energy source. If the sample collected from Onahu (Otis_Peak) is returned to Earth, analysis of the Fe-phosphates may provide new insights into ancient habitable environments on Mars.

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Journal
Nature Communications
Published
2025-07-14
DOI
https://doi.org/10.1038/s41467-025-60026-7
Citations
8
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
9.24

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article

Fe-phosphates in Jezero Crater as evidence for an ancient habitable environment on Mars

E. A. Cloutis, Nicholas J. Tosca, C. T. Adcock, W. T. Elam et al.
8 citations
Nature Communications
Planetary Science and Exploration
9.24
article

Fe-phosphates in Jezero Crater as evidence for an ancient habitable environment on Mars

E. A. Cloutis, Nicholas J. Tosca, C. T. Adcock, W. T. Elam, Mark Schmidt, Alberto González Fairén, S. J. VanBommel, Tanja Bosak, David C. Catling, J. N. Maki, Abigail C. Allwood, Abigail L. Knight, Michael W. Jones, A. H. Treiman, Y. Liu, F. M. McCubbin, Elisabeth M. Hausrath, J. A. Hurowitz, L. P. O’Neil, B. C. Clark, David A. K. Pedersen, Andrew O. Shumway, Peter S. Jørgensen, John R. Christian, K. L. Siebach, Nicolas Randazzo, T. V. Kizovski, Michael M. Tice, Morgan Leigh Cable, Christopher M. Heirwegh, Sunanda Sharma, Lawrence A. Wade, U. Wolf, Peter R. Lawson, B. P. Weiss
article en
8 citations

Abstract

Phosphorus is an essential component for life, and in-situ identification of phosphate minerals that formed in aqueous conditions directly contributes toward one of the main goals of the Mars 2020 Perseverance rover: to seek signs of ancient habitable environments. In Jezero crater, proximity science analyses within a conglomerate outcrop, "Onahu" demonstrate the presence of rare Fe<sup>3+</sup>-bearing phosphate minerals (likely metavivianite, ferrolaueite, (ferro)beraunite, and/or santabarbaraite) embedded in a carbonate-rich matrix. While Fe-phosphates have been inferred previously on Mars, this work presents the most definitive in-situ identification of martian Fe-phosphate minerals to date, using textural, chemical, spectral, and diffraction analyses of discrete green-blue grains. The Fe-phosphate minerals' textural context along with comparisons to Earth analogs suggest they likely formed after oxidation of Fe<sup>2+</sup>-phosphate vivianite, the most common Fe-phosphate in sedimentary environments on Earth, often associated with microbial activity and organics. While there is no obvious evidence of biological inputs in Onahu, if the Fe-phosphates' formation environment was similar to vivianite-rich sedimentary environments on Earth, these minerals likely originally precipitated in conditions favorable to potential martian life - in a low temperature, reducing aqueous medium with high concentrations of bio-limiting elements, and Fe-redox gradients that could provide an energy source. If the sample collected from Onahu (Otis_Peak) is returned to Earth, analysis of the Fe-phosphates may provide new insights into ancient habitable environments on Mars.

Nature CommunicationsVol. 16(1)
College of Southern Nevada (US), Space Science Institute (US), Jet Propulsion Laboratory (US), University of Nevada, Las Vegas (US), Los Alamos National Laboratory (US), University of Alberta (CA), Queensland University of Technology (AU), Brock University (CA), Carnegie Institution for Science (US), University of Washington (US), Washington University in St. Louis (US), Cornell University (US), University of Cambridge (GB), Royal Ontario Museum (CA), Centro de Astrobiología (ES), Johnson Space Center (US), Earth and Space Research (US), University of Manitoba (CA), Lunar and Planetary Institute (US), Stony Brook University (US), Massachusetts Institute of Technology (US), Rice University (US), Central Queensland University (AU), The University of Winnipeg (CA), Texas A&M University (US), Technical University of Denmark (DK)
National Aeronautics and Space Administration, California Institute of Technology, Nuclear Safety and Security Commission, Jet Propulsion Laboratory, Canadian Space Agency, Natural Sciences and Engineering Research Council of Canada
Openalex Percentile: Top 2%
Planetary Science and Exploration
9.24
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