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      Thermal metamorphism of CM chondrites: A dehydroxylation‐based peak‐temperature thermometer and implications for sample return from asteroids Ryugu and Bennu

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      Meteoritics & Planetary Science
      John Wiley and Sons Inc.

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          Abstract

          The target bodies of C‐complex asteroid sample return missions are carbonaceous chondrite‐like near‐Earth asteroids (NEAs), chosen for the abundance and scientific importance of their organic compounds and “hydrous” (including hydroxylated) minerals, such as serpentine‐group phyllosilicates. Science objectives include returning samples of pristine carbonaceous regolith from asteroids for study of the nature, history, and distribution of its constituent minerals, organic material, and other volatiles. Heating after the natural aqueous alteration that formed the abundant phyllosilicates in CM and similar carbonaceous chondrites dehydroxylated them and altered or decomposed other volumetrically minor constituents (e.g., carbonates, sulfides, organic molecules; Tonui et al. 2003, 2014). We propose a peak‐temperature thermometer based on dehydroxylation as measured by analytical totals from electron probe microanalysis (EPMA) of matrices in a number of heated and aqueously altered (but not further heated) CM chondrites. Some CM lithologies in Maribo and Sutter’s Mill do not exhibit the matrix dehydroxylation expected for surface temperatures expected from insolation of meteoroids with their known orbital perihelia. This suggests that insolated‐heated meteoroid surfaces were lost by ablation during passage through Earth’s atmosphere, and that insolation‐heated material is more likely to be encountered among returned asteroid regolith samples than in meteorites. More generally, several published lines of evidence suggest that episodic heating of some CM material, most likely by impacts, continued intermittently and locally up to billions of years after assembly and early heating of ancestral CM chondrite bodies. Mission spectroscopic measures of hydration can be used to estimate the extent of dehydroxylation, and the new dehydroxylation thermometer can be used directly to select fragments of returned samples most likely to contain less thermally altered inventories of primitive organic molecules.

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          A chemical-petrologic classification for the chondritic meteorites

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            The chemical composition of some stony meteorites

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              Carbonaceous chondrites—II. Carbonaceous chondrite phyllosilicates and light element geochemistry as indicators of parent body processes and surface conditions

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                Author and article information

                Contributors
                velbel@msu.edu
                Journal
                Meteorit Planet Sci
                Meteorit Planet Sci
                10.1111/(ISSN)1945-5100
                MAPS
                Meteoritics & Planetary Science
                John Wiley and Sons Inc. (Hoboken )
                1086-9379
                1945-5100
                08 April 2021
                March 2021
                : 56
                : 3 ( doiID: 10.1111/maps.v56.3 )
                : 546-585
                Affiliations
                [ 1 ] Department of Earth and Environmental Sciences Michigan State University 288 Farm Lane, Room 207, Natural Sciences Building East Lansing Michigan 48824–1115 USA
                [ 2 ] Division of Meteorites Department of Mineral Sciences National Museum of Natural History Smithsonian Institution Washington District of Columbia 20013–7012 USA
                [ 3 ] X12 Astromaterials Research and Exploration Science NASA Johnson Space Center Houston Texas 77058 USA
                Author notes
                [*] [* ] Corresponding author. E‐mail: velbel@ 123456msu.edu

                Author information
                https://orcid.org/0000-0002-9108-8153
                https://orcid.org/0000-0002-3181-1303
                Article
                MAPS13636
                10.1111/maps.13636
                8252763
                34262245
                f8e0927f-06d3-42af-86c9-1f4aee6e0b39
                © 2021 The Authors. Meteoritics & Planetary Science published by Wiley Periodicals LLC on behalf of The Meteoritical Society.

                This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc-nd/4.0/ License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.

                History
                : 17 September 2019
                : 17 January 2021
                Page count
                Figures: 2, Tables: 5, Pages: 40, Words: 34350
                Funding
                Funded by: Michigan Space Grant Consortium , open-funder-registry 10.13039/100005746;
                Award ID: NNX15AJ20H
                Funded by: National Aeronautics and Space Administration , open-funder-registry 10.13039/100000104;
                Award ID: 80NSSC18K0593
                Categories
                Article
                Articles
                Custom metadata
                2.0
                March 2021
                Converter:WILEY_ML3GV2_TO_JATSPMC version:6.0.4 mode:remove_FC converted:02.07.2021

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