From hydrated silica to quartz: Potential hydrothermal precipitates found in Jezero crater, Mars
Pierre Beck, O. Beyssac, E. Dehouck, S. A. Bernard, Maxime Pineau, Lucia Mandon, Clément Royer, Elise Clavé, Susanne Schröder, O. Forni, Raymond Francis, N. Mangold, C. C. Bedford, Adrian Broz, E. A. Cloutis, J. R. Johnson, F. Poulet, Thierry Fouchet, Cathy Quantin‐Nataf, C. Pilorget, W. Rapin, Pierre‐Yves Meslin, T. S. J. Gabriel, Gorka Arana, Juan Manuel Madariaga, A. J. Brown, S. Maurice, S. M. Clegg, O. Gasnault, A. Cousin, R. C. Wiens
Abstract
• Silica-rich float rocks were discovered by Perseverance. • Quartz, chalcedony and opal were found. • These rocks were part of an ancient hydrothermal system. • If found by the rover, the source deposit is a high-value target for sampling. On Earth, silica-rich phases from opal to quartz are important indicators and tracers of geological processes. Hydrated silica, such as opal, is a particularly good matrix for the preservation of molecular and macroscopic biosignatures. Cherts, a type of silica-dominated rocks, provide a unique archive of ancient terrestrial life while quartz is the emblematic mineral of the Earth's continental crust. On Mars, hydrated silica has been detected in several locations based on remote sensing and rover-based studies. In the present article we report on the detection of cobbles made of hydrated silica (opal or chalcedony), as well as well-crystallized quartz. These detections were made with the SuperCam instrument onboard Perseverance (Mars 2020 mission), using a combination of LIBS, infrared and Raman spectroscopy. Quartz-dominated stones are detected unambiguously for the first time on the Martian surface, and based on grain size and crystallinity are proposed to be of hydrothermal origin. Although these rocks were all found as float, we propose that these detections are part of a common hydrothermal system, and represent different depths / temperatures of precipitation. This attests that hydrothermal processes were active in and around Jezero crater, possibly triggered by the Jezero crater-forming impact. These silica-rich rocks, in particular opaline silica, are very promising targets for sampling and return to Earth given their high biosignature preservation potential.