Petrological Traverse of the Olivine Cumulate Séítah Formation at Jezero Crater, Mars: A Perspective From SuperCam Onboard Perseverance
Olivier Beyssac, O. Forni, A. Cousin, Arya Udry, Linda C. Kah, Lucia Mandon, O. E. Clavé, Yang Liu, F. Poulet, Cathy Quantin Nataf, O. Gasnault, J. R. Johnson, Karim Benzerara, Pierre Beck, E. Dehouck, N. Mangold, César Álvarez-Llamas, R. B. Anderson, Gorka Arana, Robert Barnes, Sylvain Bernard, Tanja Bosak, A. J. Brown, Kepa Castro, Baptiste Chide, S. M. Clegg, E. A. Cloutis, Thierry Fouchet, T. S. J. Gabriel, Sanjeev Gupta, Gaétan Lacombe, J. Lasue, Stéphane Le Mouëlic, G. López-Reyes, Juan Manuel Madariaga, F. M. McCubbin, S. M. McLennan, J. A. Manrique, Pierre‐Yves Meslin, Franck Montmessin, Jorge I. Núñez, A. Ollila, Amanda Ostwald, P. Pilleri, P. Pinet, Clément Royer, Shiv K. Sharma, Susanne Schröder, Justin I. Simon, Michael J. Toplis, Marco Veneranda, Peter A. Willis, S. Maurice, R. C. Wiens, The SuperCam Team
Abstract
Abstract Séítah is the stratigraphically lowest formation visited by Perseverance in the Jezero crater floor. We present the data obtained by SuperCam: texture by imagery, chemistry by Laser‐Induced Breakdown Spectroscopy, and mineralogy by Supercam Visible and Infrared reflectance and Raman spectroscopy. The Séítah formation consists of igneous, weakly altered rocks dominated by millimeter‐sized grains of olivine with the presence of low‐Ca and high‐Ca pyroxenes, and other primary minerals (e.g., plagioclase, Cr‐Fe‐Ti oxides, phosphates). Along a ∼140 m long section in Séítah, SuperCam analyses showed evidence of geochemical and mineralogical variations, from the contact with the overlying Máaz formation, going deeper in the formation. Bulk rock and olivine Mg#, grain size, olivine content increase gradually further from the contact. Along the section, olivine Mg# is not in equilibrium with the bulk rock Mg#, indicating local olivine accumulation. These observations are consistent with Séítah being the deep ultramafic member of a cumulate series derived from the fractional crystallization and slow cooling of the parent magma at depth. Possible magmatic processes and exhumation mechanisms of Séítah are discussed. Séítah rocks show some affinity with some rocks at Gusev crater, and with some Martian meteorites suggesting that such rocks are not rare on the surface of Mars. Séítah is part of the Nili Fossae regional olivine‐carbonate unit observed from orbit. Future exploration of Perseverance on the rim and outside of the crater will help determine if the observations from the crater floor can be extrapolated to the whole unit or if this unit is composed of distinct sub‐units with various origins.