Multiple Episodes of Fluid Alteration in Jezero Crater Indicated by MIST Mineral Identifications in PIXL XRF Data from the First 1100 Sols of the Mars 2020 Mission

The Mineral Identification by Stoichiometry (MIST) algorithm can identify mineral species in geochemical datasets. MIST is applied to X-ray fluorescence (XRF) chemical analyses from the Planetary Instrument for X-ray Lithochemistry (PIXL) on the Mars 2020 Perseverance rover to identify mineral phases in abraded rock targets at Jezero crater. We used a Monte Carlo error propagation technique to assess confidence in the results. Our study reports 24 high-confidence mineral phases from the first 1100 sols of Perseverance’s traverse. Primary mineral groups include plagioclase, pyroxene, and olivine, in agreement with previously published results, and support an (ultra)mafic rock source. Additionally, MIST identified a range of phyllosilicate for minerals, including nontronite, saponite, hisingerite, greenalite, minnesotaite, and sepiolite; identification of such alteration phases is essential for constraining the aqueous alteration historyof Jezero’s rocks. An initial survey of the reported phases suggests multiple, distinct stages of fluid alteration in Jezero’s history: high temperature and acidic, moderate temperature and circumneutral, and later stage ambient alkaline conditions. MIST results from PIXL data help determine rocks of interest on Mars’ surface for investigation by Perseverance and will also be important for informing analysis of samples when returned to Earth.