The Tarda Meteorite: A Window into the Formation of D-type Asteroids
Dynamic models of solar system evolution suggest that D-type asteroids formed beyond Saturn's orbit and represent invaluable witnesses of the prevailing conditions in the outer solar system. Here, we report a comprehensive petrographic and isotopic characterization of the carbonaceous chondrite...
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ftarchimer:oai:archimer.ifremer.fr:80884 2023-05-15T18:30:04+02:00 The Tarda Meteorite: A Window into the Formation of D-type Asteroids Marrocchi, Yves Avice, Guillaume Barrat, Jean-alix 2021-05 application/pdf https://archimer.ifremer.fr/doc/00697/80884/84618.pdf https://doi.org/10.3847/2041-8213/abfaa3 https://archimer.ifremer.fr/doc/00697/80884/ eng eng American Astronomical Society https://archimer.ifremer.fr/doc/00697/80884/84618.pdf doi:10.3847/2041-8213/abfaa3 https://archimer.ifremer.fr/doc/00697/80884/ info:eu-repo/semantics/openAccess restricted use Astrophysical Journal Letters (2041-8205) (American Astronomical Society), 2021-05 , Vol. 913 , N. 1 , P. L9 (8p.) text Publication info:eu-repo/semantics/article 2021 ftarchimer https://doi.org/10.3847/2041-8213/abfaa3 2022-05-24T22:50:02Z Dynamic models of solar system evolution suggest that D-type asteroids formed beyond Saturn's orbit and represent invaluable witnesses of the prevailing conditions in the outer solar system. Here, we report a comprehensive petrographic and isotopic characterization of the carbonaceous chondrite Tarda, a recent fall recovered in the Moroccan Sahara. We show that Tarda shares strong similarities with the D-type-derived chondrite Tagish Lake, implying that Tarda represents a rare sample of D-type asteroids. Both Tarda and Tagish Lake are characterized by the presence of rare 16O-rich chondrules and chondrule fragments, high C/H ratios, and enrichments in deuterium, 15N, and 13C. By combining our results with literature data on carbonaceous chondrites related to C-type asteroids, we show that the outer solar system 4.56 Gy ago was characterized by large-scale oxygen isotopic homogeneities in (i) the water–ice grains accreted by asteroids and (ii) the gas controlling the formation of FeO-poor chondrules. Conversely, the zone in which D-type asteroids accreted was significantly enriched in deuterium relative to the formation regions of C-type asteroids, features likely inherited from unprocessed, D-rich, molecular-cloud materials. Article in Journal/Newspaper Tagish Archimer (Archive Institutionnelle de l'Ifremer - Institut français de recherche pour l'exploitation de la mer) Tagish ENVELOPE(-134.272,-134.272,60.313,60.313) Tagish Lake ENVELOPE(-134.233,-134.233,59.717,59.717) The Astrophysical Journal Letters 913 1 L9 |
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Open Polar |
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Archimer (Archive Institutionnelle de l'Ifremer - Institut français de recherche pour l'exploitation de la mer) |
op_collection_id |
ftarchimer |
language |
English |
description |
Dynamic models of solar system evolution suggest that D-type asteroids formed beyond Saturn's orbit and represent invaluable witnesses of the prevailing conditions in the outer solar system. Here, we report a comprehensive petrographic and isotopic characterization of the carbonaceous chondrite Tarda, a recent fall recovered in the Moroccan Sahara. We show that Tarda shares strong similarities with the D-type-derived chondrite Tagish Lake, implying that Tarda represents a rare sample of D-type asteroids. Both Tarda and Tagish Lake are characterized by the presence of rare 16O-rich chondrules and chondrule fragments, high C/H ratios, and enrichments in deuterium, 15N, and 13C. By combining our results with literature data on carbonaceous chondrites related to C-type asteroids, we show that the outer solar system 4.56 Gy ago was characterized by large-scale oxygen isotopic homogeneities in (i) the water–ice grains accreted by asteroids and (ii) the gas controlling the formation of FeO-poor chondrules. Conversely, the zone in which D-type asteroids accreted was significantly enriched in deuterium relative to the formation regions of C-type asteroids, features likely inherited from unprocessed, D-rich, molecular-cloud materials. |
format |
Article in Journal/Newspaper |
author |
Marrocchi, Yves Avice, Guillaume Barrat, Jean-alix |
spellingShingle |
Marrocchi, Yves Avice, Guillaume Barrat, Jean-alix The Tarda Meteorite: A Window into the Formation of D-type Asteroids |
author_facet |
Marrocchi, Yves Avice, Guillaume Barrat, Jean-alix |
author_sort |
Marrocchi, Yves |
title |
The Tarda Meteorite: A Window into the Formation of D-type Asteroids |
title_short |
The Tarda Meteorite: A Window into the Formation of D-type Asteroids |
title_full |
The Tarda Meteorite: A Window into the Formation of D-type Asteroids |
title_fullStr |
The Tarda Meteorite: A Window into the Formation of D-type Asteroids |
title_full_unstemmed |
The Tarda Meteorite: A Window into the Formation of D-type Asteroids |
title_sort |
tarda meteorite: a window into the formation of d-type asteroids |
publisher |
American Astronomical Society |
publishDate |
2021 |
url |
https://archimer.ifremer.fr/doc/00697/80884/84618.pdf https://doi.org/10.3847/2041-8213/abfaa3 https://archimer.ifremer.fr/doc/00697/80884/ |
long_lat |
ENVELOPE(-134.272,-134.272,60.313,60.313) ENVELOPE(-134.233,-134.233,59.717,59.717) |
geographic |
Tagish Tagish Lake |
geographic_facet |
Tagish Tagish Lake |
genre |
Tagish |
genre_facet |
Tagish |
op_source |
Astrophysical Journal Letters (2041-8205) (American Astronomical Society), 2021-05 , Vol. 913 , N. 1 , P. L9 (8p.) |
op_relation |
https://archimer.ifremer.fr/doc/00697/80884/84618.pdf doi:10.3847/2041-8213/abfaa3 https://archimer.ifremer.fr/doc/00697/80884/ |
op_rights |
info:eu-repo/semantics/openAccess restricted use |
op_doi |
https://doi.org/10.3847/2041-8213/abfaa3 |
container_title |
The Astrophysical Journal Letters |
container_volume |
913 |
container_issue |
1 |
container_start_page |
L9 |
_version_ |
1766213542250283008 |