Alteration history of Séítah formation rocks inferred by PIXL x-ray fluorescence, x-ray diffraction, and multispectral imaging on Mars
Michael M. Tice, J. A. Hurowitz, Abigail C. Allwood, Michael W. Jones, Brendan J. Orenstein, Scott Davidoff, Austin P. Wright, David A. K. Pedersen, Jesper Henneke, Nicholas J. Tosca, Kelsey Moore, B. C. Clark, S. M. McLennan, David Flannery, A. Steele, A. J. Brown, María‐Paz Zorzano, Keyron Hickman‐Lewis, Yang Liu, S. J. VanBommel, M. E. Schmidt, T. V. Kizovski, A. H. Treiman, L. P. O’Neil, Alberto González Fairén, David L. Shuster, Sanjeev Gupta, The PIXL Team
Abstract
Collocated crystal sizes and mineral identities are critical for interpreting textural relationships in rocks and testing geological hypotheses, but it has been previously impossible to unambiguously constrain these properties using in situ instruments on Mars rovers. Here, we demonstrate that diffracted and fluoresced x-rays detected by the PIXL instrument (an x-ray fluorescence microscope on the Perseverance rover) provide information about the presence or absence of coherent crystalline domains in various minerals. X-ray analysis and multispectral imaging of rocks from the Séítah formation on the floor of Jezero crater shows that they were emplaced as coarsely crystalline igneous phases. Olivine grains were then partially dissolved and filled by finely crystalline or amorphous secondary silicate, carbonate, sulfate, and chloride/oxychlorine minerals. These results support the hypothesis that Séítah formation rocks represent olivine cumulates altered by fluids far from chemical equilibrium at low water-rock ratios.