Abrasion Patch Dehydration Experiment at Bright Angel, Jezero Crater, Using SuperCam Onboard the Mars 2020 Perseverance Rover

Abstract Investigating the stability of hydrated minerals is integral for examining the preservation of rocks for potential Mars Sample Return and has major implications for models that use rover‐based observations to quantify Mars' global water budget. The Mars 2020 Perseverance rover produces abrasion patches to investigate fresh rock surfaces at Jezero crater, Mars. However, due to operational constraints, the full analysis process typically takes several martian days (sols), and freshly exposed hydrated minerals may dehydrate upon atmospheric exposure between abrasion patch creation and their analyses. To assess the potential for short‐term dehydration, the SuperCam instrument conducted the first in situ rover‐based dehydration experiment on rock exposures of the “Bright Angel formation.” The SuperCam and SHERLOC rover instruments indicated that the primary mineral hydration phases were Fe‐hydroxides, Ca‐sulfates such as bassanite (mixed with anhydrite), with possible minor contributions from non‐interlayer‐water phyllosilicates (e.g., hydroxyl‐bearing only). The experiment involved a four‐sol sequence of observations on the Steamboat Mountain abrasion patch, beginning just 22 min after abrasion. Dehydration was assessed by tracking changes in the 1.93 μm H 2 O absorption feature, which is sensitive to structural, absorbed, and adsorbed water. No significant changes in hydration were observed over the 93 hr, suggesting that the exposed minerals were already in a low hydration state and/or exhibit high stability under current martian surface conditions. These findings imply bulk rocks with low hydration and high stability minerals may not dehydrate upon exposure to the modern martian atmosphere on short time scales, consistent with predictions from laboratory simulations of Mars‐like environments.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2025-12-01
DOI
https://doi.org/10.1029/2025je009243
Citations
1
Primary Topic
Planetary Science and Exploration
Type
article
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article

Abrasion Patch Dehydration Experiment at Bright Angel, Jezero Crater, Using SuperCam Onboard the Mars 2020 Perseverance Rover

E. A. Cloutis, Jason Van Beek, E. Dehouck, J. A. Rodríguez‐Manfredi et al.
1 citations
Journal of Geophysical Research Planets
Planetary Science and Exploration
1.15
article

Abrasion Patch Dehydration Experiment at Bright Angel, Jezero Crater, Using SuperCam Onboard the Mars 2020 Perseverance Rover

E. A. Cloutis, Jason Van Beek, E. Dehouck, J. A. Rodríguez‐Manfredi, Lucia Mandon, Clément Royer, Kyle Uckert, C. C. Bedford, K. P. Hand, F. Poulet, Sandra Siljeström, Susanne Schröder, Elise Clavé, Á. Vicente‐Retortillo, Stephanie Connell, Thierry Fouchet, Adrian Broz, Teresa Fornaro, Andrew Alberini, D. M. Applin, R. C. Wiens, T. Nelson, Kathryn M. Stack, Pierre Beck, A. Cousin, Germán Martínez, Alexander Jones
article en
1 citations

Abstract

Abstract Investigating the stability of hydrated minerals is integral for examining the preservation of rocks for potential Mars Sample Return and has major implications for models that use rover‐based observations to quantify Mars' global water budget. The Mars 2020 Perseverance rover produces abrasion patches to investigate fresh rock surfaces at Jezero crater, Mars. However, due to operational constraints, the full analysis process typically takes several martian days (sols), and freshly exposed hydrated minerals may dehydrate upon atmospheric exposure between abrasion patch creation and their analyses. To assess the potential for short‐term dehydration, the SuperCam instrument conducted the first in situ rover‐based dehydration experiment on rock exposures of the “Bright Angel formation.” The SuperCam and SHERLOC rover instruments indicated that the primary mineral hydration phases were Fe‐hydroxides, Ca‐sulfates such as bassanite (mixed with anhydrite), with possible minor contributions from non‐interlayer‐water phyllosilicates (e.g., hydroxyl‐bearing only). The experiment involved a four‐sol sequence of observations on the Steamboat Mountain abrasion patch, beginning just 22 min after abrasion. Dehydration was assessed by tracking changes in the 1.93 μm H 2 O absorption feature, which is sensitive to structural, absorbed, and adsorbed water. No significant changes in hydration were observed over the 93 hr, suggesting that the exposed minerals were already in a low hydration state and/or exhibit high stability under current martian surface conditions. These findings imply bulk rocks with low hydration and high stability minerals may not dehydrate upon exposure to the modern martian atmosphere on short time scales, consistent with predictions from laboratory simulations of Mars‐like environments.

Journal of Geophysical Research PlanetsVol. 130(12)
Université Claude Bernard Lyon 1 (FR), École Normale Supérieure de Lyon (FR), Centre National de la Recherche Scientifique (FR), Jet Propulsion Laboratory (US), Los Alamos National Laboratory (US), Université Toulouse III - Paul Sabatier (FR), Université Paris Cité (FR), Purdue University West Lafayette (US), Université Paris-Saclay (FR), Arcetri Astrophysical Observatory (IT), Observatoire de Paris (FR), RISE Research Institutes of Sweden (SE), Johns Hopkins University Applied Physics Laboratory (US), Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE), Sorbonne Université (FR), Sorbonne Paris Cité (FR), Centro de Astrobiología (ES), Institut de Recherche en Astrophysique et Planétologie (FR), Imperial College London (GB), The University of Winnipeg (CA), Université Grenoble Alpes (FR)
Openalex Percentile: Top 14%
Planetary Science and Exploration
1.15
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