Alteration of a Mantle‐Derived Dunite Boulder in Jezero Crater, Mars
E. L. Moreland, M. Bramble, K. L. Siebach, A. C. Pascuzzo, M. Morris, S. J. VanBommel, M. Jones, S. Siljeström, A. Srivastava, A. H. Treiman, J. HurowitzAbstract
In 2023, the Mars 2020 Perseverance rover explored the youngest preserved deposits on the Western fan of Jezero crater, Mars: a field of meter‐scale boulders dispersed above the previously explored sandstone and siltstone units. Reflectance spectra of the boulders delineated two classes, one olivine‐bearing and one pyroxene‐bearing. A representative boulder from each class was analyzed; here, we present proximity data from the olivine‐rich target, Falcon Lake, revealing a magnesian dunite (Fo 74 ). Such magnesian dunite is distinct from other igneous materials observed in Jezero and consistent with crystallization from a mantle‐derived partial melt. Micron and mm‐scale secondary minerals, identified on the abraded patch of Falcon Lake, include Mg‐serpentine, Fe‐Mg carbonate, and Mg,Fe sulfate. This alteration sequence records sequential precipitation from a single evolving fluid, and the coexistence of disequilibrium sulfate and siderite represents a microscale analog to planet‐wide associations and detections of carbonates and sulfates.