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Overview of the Morphology and Chemistry of Diagenetic Features in the Clay-Rich Glen Torridon Unit of Gale Crater, Mars

Authors :
Patrick J. Gasda
Jade Comellas
Ari Essunfeld
Debarati Das
Alexander B. Bryk
Erwin Dehouck
Susanne P. Schwenzer
Laura Crossey
Kenneth Herkenhoff
Jeffrey R. Johnson
Horton Newsom
Nina L. Lanza
William Rapin
Walter Goetz
Pierre‐Yves Meslin
John C. Bridges
Ryan Anderson
Gael David
Stuart M. R. Turner
Michael T. Thorpe
Linda Kah
Jens Frydenvang
Rachel Kronyak
Gwénaël Caravaca
Ann Ollila
Stéphane Le Mouélic
Matthew Nellessen
Megan Hoffman
Deirdra Fey
Anges Cousin
Roger C. Wiens
Samuel M. Clegg
Sylvestre Maurice
Olivier Gasnault
Dorothea Delapp
Adriana Reyes‐Newell
Los Alamos National Laboratory (LANL)
McGill University = Université McGill [Montréal, Canada]
University of California [Berkeley] (UC Berkeley)
University of California (UC)
The Open University [Milton Keynes] (OU)
The University of New Mexico [Albuquerque]
US Geological Survey [Flagstaff]
United States Geological Survey [Reston] (USGS)
Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL)
Institut de recherche en astrophysique et planétologie (IRAP)
Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS)
Max-Planck-Gesellschaft
University of Leicester
Texas State University
NASA Johnson Space Center (JSC)
NASA
The University of Tennessee [Knoxville]
Globe Institute
Faculty of Health and Medical Sciences
University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)
Jet Propulsion Laboratory (JPL)
NASA-California Institute of Technology (CALTECH)
Laboratoire de Planétologie et Géosciences [UMR_C 6112] (LPG)
Université d'Angers (UA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST)
Nantes Université - pôle Sciences et technologie
Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie
Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)
Malin Space Science Systems (MSSS)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Max Planck Institute for Solar System Research (MPS)
Laboratoire de Planétologie et Géosciences - Angers (LPG-ANGERS)
Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Université d'Angers (UA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST)
Source :
Journal of Geophysical Research (Planets), Journal of Geophysical Research. Planets, Journal of Geophysical Research. Planets, 2022, The Curiosity Rover's Investigation of Glen Torridon and the Surrounding Area, 127 (12), pp.e2021JE007097. ⟨10.1029/2021JE007097⟩, Gasda, P J, Comellas, J, Essunfeld, A, Das, D, Bryk, A B, Dehouck, E, Schwenzer, S P, Crossey, L, Herkenhoff, K, Johnson, J R, Newsom, H, Lanza, N L, Rapin, W, Goetz, W, Meslin, P-Y, Bridges, J C, Anderson, R, David, G, Turner, S M R, Thorpe, M T, Kah, L, Frydenvang, J, Kronyak, R, Caravaca, G, Ollila, A, Le Mouélic, S, Nellessen, M, Hoffman, M, Fey, D, Cousin, A, Wiens, R C, Clegg, S M, Maurice, S, Gasnault, O, Delapp, D & Reyes-Newell, A 2022, ' Overview of the Morphology and Chemistry of Diagenetic Features in the Clay-Rich Glen Torridon Unit of Gale Crater, Mars ', Journal of Geophysical Research: Planets, vol. 127, no. 12, e2021JE007097 . https://doi.org/10.1029/2021JE007097, Journal of Geophysical Research. Planets, In press, ⟨10.1029/2021JE007097⟩
Publication Year :
2022

Abstract

International audience; The clay-rich Glen Torridon region of Gale crater, Mars, was explored between sols 2300 and 3007. Here, we analyzed the diagenetic features observed by Curiosity, including veins, cements, nodules, and nodular bedrock, using the ChemCam, Mastcam, and Mars Hand Lens Imager instruments. We discovered many diagenetic features in Glen Torridon, including dark-toned iron- and manganese-rich veins, magnesium- and fluorine-rich linear features, Ca-sulfate cemented bedrock, manganese-rich nodules, and iron-rich strata. We have characterized the chemistry and morphology of these features, which are most widespread in the higher stratigraphic members in Glen Torridon, and exhibit a wide range of chemistries. These discoveries are strong evidence for multiple generations of fluids from multiple chemical endmembers that likely underwent redox reactions to form some of these features. In a few cases, we may be able to use mineralogy and chemistry to constrain formation conditions of the diagenetic features. For example, the dark-toned veins likely formed in warmer, highly alkaline, and highly reducing conditions, while manganese-rich nodules likely formed in oxidizing and circumneutral conditions. We also hypothesize that an initial enrichment of soluble elements, including fluorine, occurred during hydrothermal alteration early in Gale crater history to account for elemental enrichment in nodules and veins. The presence of redox-active elements, including Fe and Mn, and elements required for life, including P and S, in these fluids is strong evidence for habitability of Gale crater groundwater. Hydrothermal alteration also has interesting implications for prebiotic chemistry during the earliest stages of the crater’s evolution and early Mars.

Details

ISSN :
21699100 and 21699097
Database :
OpenAIRE
Journal :
Journal of Geophysical Research (Planets), Journal of Geophysical Research. Planets, Journal of Geophysical Research. Planets, 2022, The Curiosity Rover's Investigation of Glen Torridon and the Surrounding Area, 127 (12), pp.e2021JE007097. ⟨10.1029/2021JE007097⟩, Gasda, P J, Comellas, J, Essunfeld, A, Das, D, Bryk, A B, Dehouck, E, Schwenzer, S P, Crossey, L, Herkenhoff, K, Johnson, J R, Newsom, H, Lanza, N L, Rapin, W, Goetz, W, Meslin, P-Y, Bridges, J C, Anderson, R, David, G, Turner, S M R, Thorpe, M T, Kah, L, Frydenvang, J, Kronyak, R, Caravaca, G, Ollila, A, Le Mouélic, S, Nellessen, M, Hoffman, M, Fey, D, Cousin, A, Wiens, R C, Clegg, S M, Maurice, S, Gasnault, O, Delapp, D & Reyes-Newell, A 2022, ' Overview of the Morphology and Chemistry of Diagenetic Features in the Clay-Rich Glen Torridon Unit of Gale Crater, Mars ', Journal of Geophysical Research: Planets, vol. 127, no. 12, e2021JE007097 . https://doi.org/10.1029/2021JE007097, Journal of Geophysical Research. Planets, In press, ⟨10.1029/2021JE007097⟩
Accession number :
edsair.doi.dedup.....624562cbd6e8097311fc9851ff929451
Full Text :
https://doi.org/10.1029/2021JE007097⟩