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Research Article

Insights into the origin of carbonaceous chondrite organics from their triple oxygen isotope composition

View ORCID ProfileRomain Tartèse, Marc Chaussidon, Andrey Gurenko, Frédéric Delarue, and François Robert
  1. aSchool of Earth and Environmental Sciences, The University of Manchester, Manchester M13 9PL, United Kingdom;
  2. bInstitut de Physique du Globe de Paris, Université Sorbonne-Paris-Cité, Université Paris Diderot, CNRS UMR 7154, F-75238 Paris, France;
  3. cCentre de Recherches Pétrographiques et Géochimiques, UMR 7358, Université de Lorraine, F-54501 Vandoeuvre-lès-Nancy, France;
  4. dSorbonne Université, Université Pierre-et-Marie-Curie, CNRS, École Pratique des Hautes Etudes, Paris Sciences et Lettres, UMR 7619 Milieux Environnementaux, Transferts et Interactions dans les Hydrosystèmes et les Sols, F-75005 Paris, France;
  5. eInstitut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Muséum National d’Histoire Naturelle, Sorbonne Universités, CNRS, Université Pierre-et-Marie-Curie, and Institut de Recherche pour le Développement, F-75005 Paris, France

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PNAS August 21, 2018 115 (34) 8535-8540; first published August 6, 2018; https://doi.org/10.1073/pnas.1808101115
Romain Tartèse
aSchool of Earth and Environmental Sciences, The University of Manchester, Manchester M13 9PL, United Kingdom;
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  • ORCID record for Romain Tartèse
  • For correspondence: romain.tartese@manchester.ac.uk
Marc Chaussidon
bInstitut de Physique du Globe de Paris, Université Sorbonne-Paris-Cité, Université Paris Diderot, CNRS UMR 7154, F-75238 Paris, France;
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Andrey Gurenko
cCentre de Recherches Pétrographiques et Géochimiques, UMR 7358, Université de Lorraine, F-54501 Vandoeuvre-lès-Nancy, France;
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Frédéric Delarue
dSorbonne Université, Université Pierre-et-Marie-Curie, CNRS, École Pratique des Hautes Etudes, Paris Sciences et Lettres, UMR 7619 Milieux Environnementaux, Transferts et Interactions dans les Hydrosystèmes et les Sols, F-75005 Paris, France;
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François Robert
eInstitut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Muséum National d’Histoire Naturelle, Sorbonne Universités, CNRS, Université Pierre-et-Marie-Curie, and Institut de Recherche pour le Développement, F-75005 Paris, France
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  1. Edited by Mark H. Thiemens, University of California, San Diego, La Jolla, CA, and approved July 12, 2018 (received for review May 10, 2018)

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    Fig. 1.

    δ17,18O values obtained in Orgueil, Murchison, and Cold Bokkeveld IOM residues. The terrestrial fractionation line (TFL), the carbonaceous chondrite anhydrous mineral line (CCAM) (19), and the Young and Russell line (Y&R) (20) are also represented.

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    Fig. 2.

    NanoSIMS images showing the distribution of 12C14N, 16O, 56Fe16O, and 28Si secondary ion species in Murchison and Orgueil IOM acid maceration residues. White and cyan arrows indicate higher 56Fe16O and 28Si intensities, respectively.

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    Fig. 3.

    Examples of the ROIs defined on 16O ion images for one analysis each of Murchison and Orgueil acid residues. ROI#3 (Left) corresponds to intermediate O intensity, ROI#4 (Center) corresponds to O hot spots, and ROI#5 (Right) corresponds to pure IOM (see text for details).

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    Fig. 4.

    Calculated O isotope values for mixed compositions between the estimated IOM δ17,18O values (gray stars) in (A) Murchison and (B) Orgueil acid residues and the most negative δ17,18O values measured in mineral phases in both Murchison (approximately −40‰ for spinel; ref. 21) and Orgueil (approximately −10‰ for olivine; ref. 22) (dark gray hexagons). White dots represent 10% mixing intervals, and 20% mixing intervals are given on the diagrams from 0 to 100% mineral contribution.

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    Fig. 5.

    O isotope compositions measured by L-SIMS on IOM residues isolated from the Orgueil and Murchison carbonaceous chondrites. The terrestrial fractionation line (TFL), the CCAM line, and the Y&R line are also represented, together with the O isotope compositions of the Sun (17), of CI and CM chondrite components (bulk, matrix, and anhydrous silicates; refs. 21, 22, 26, and 27), of carbonaceous chondrite Ca- and Al-rich inclusions (30–32), chondrules (33–37), and carbonates (38). Estimates for the O isotope composition of CM chondrite primordial water (HW1 and HW2) are from ref. 27 for HW1 and ref. 38 for HW2.

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Insights into the origin of carbonaceous chondrite organics from their triple oxygen isotope composition
Romain Tartèse, Marc Chaussidon, Andrey Gurenko, Frédéric Delarue, François Robert
Proceedings of the National Academy of Sciences Aug 2018, 115 (34) 8535-8540; DOI: 10.1073/pnas.1808101115

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Insights into the origin of carbonaceous chondrite organics from their triple oxygen isotope composition
Romain Tartèse, Marc Chaussidon, Andrey Gurenko, Frédéric Delarue, François Robert
Proceedings of the National Academy of Sciences Aug 2018, 115 (34) 8535-8540; DOI: 10.1073/pnas.1808101115
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Proceedings of the National Academy of Sciences: 115 (34)
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