THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE

thesis of Manuel Petitat at the Laboratoire de Minéralogie et de Cosmochimie du Muséum National d’Histoire Naturelle, Paris and was supported by the Origin network (Marie Curie European Fellowship) International audience Early solar materials bear a variety of isotopic anomalies that reflect composi...

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Published in:The Astrophysical Journal
Main Authors: Petitat, M., Birck, J.-L., Luu, T., H, Gounelle, M.
Other Authors: Laboratoire de Minéralogie et Cosmochimie du Muséum (LMCM), Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique du Globe de Paris (IPGP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS), Centre de Recherches Pétrographiques et Géochimiques (CRPG), Institut national des sciences de l'Univers (INSU - CNRS)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2011
Subjects:
Online Access:https://insu.hal.science/insu-02163323
https://insu.hal.science/insu-02163323/document
https://insu.hal.science/insu-02163323/file/Petitat_2011_ApJ_736_23.pdf
https://doi.org/10.1088/0004-637X/736/1/23
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spelling ftinsu:oai:HAL:insu-02163323v1 2023-10-09T21:56:11+02:00 THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE Petitat, M. Birck, J.-L. Luu, T., H Gounelle, M. Laboratoire de Minéralogie et Cosmochimie du Muséum (LMCM) Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS) Institut de Physique du Globe de Paris (IPGP) Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS) Centre de Recherches Pétrographiques et Géochimiques (CRPG) Institut national des sciences de l'Univers (INSU - CNRS)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS) 2011 https://insu.hal.science/insu-02163323 https://insu.hal.science/insu-02163323/document https://insu.hal.science/insu-02163323/file/Petitat_2011_ApJ_736_23.pdf https://doi.org/10.1088/0004-637X/736/1/23 en eng HAL CCSD American Astronomical Society info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/736/1/23 insu-02163323 https://insu.hal.science/insu-02163323 https://insu.hal.science/insu-02163323/document https://insu.hal.science/insu-02163323/file/Petitat_2011_ApJ_736_23.pdf doi:10.1088/0004-637X/736/1/23 info:eu-repo/semantics/OpenAccess ISSN: 0004-637X EISSN: 1538-4357 The Astrophysical Journal https://insu.hal.science/insu-02163323 The Astrophysical Journal, 2011, 736 (1), pp.23. ⟨10.1088/0004-637X/736/1/23⟩ meteors meteorites meteoroids nucleosynthesis abundances nuclear reactions supernovae: general [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] [SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry info:eu-repo/semantics/article Journal articles 2011 ftinsu https://doi.org/10.1088/0004-637X/736/1/23 2023-09-13T16:32:17Z thesis of Manuel Petitat at the Laboratoire de Minéralogie et de Cosmochimie du Muséum National d’Histoire Naturelle, Paris and was supported by the Origin network (Marie Curie European Fellowship) International audience Early solar materials bear a variety of isotopic anomalies that reflect compositional differences deriving from distinct stellar nucleosynthetic processes. As shown in previous studies, the stepwise dissolution with increasing acid strengths of bulk rock carbonaceous chondrites liberates Cr with both excesses and deficits in 53 Cr and 54 Cr relative to the terrestrial standard. The magnitude of the 54 Cr variations within a meteorite decreases in the sequence CI1 > CR2 > CM2 > CV3 > CO3 > CK4 and correlates with the degree of metamorphism of each carbonaceous chondrite class. This study shows that the Tagish Lake meteorite presents the highest excesses in 54 Cr ever measured in a bulk silicate phase. According to this study, the Tagish Lake meteorite is composed of the least re-equilibrated material known at this time. The magnitude of 54 Cr variation decreases now in the following sequence: Tagish Lake (ungrouped CI2) > Orgueil (CI1) > Murchison (CM2) > Allende (CV2). Moreover, this study shows that excesses in 53 Cr relative to Earth can be interpreted as representing the extent of aqueous alteration on meteorite parent bodies. Finally, the high 54 Cr anomalies measured in this meteorite make Tagish Lake one of the major targets to decipher the host of these anomalies. Article in Journal/Newspaper Tagish Institut national des sciences de l'Univers: HAL-INSU Murchison ENVELOPE(144.250,144.250,-67.317,-67.317) Tagish ENVELOPE(-134.272,-134.272,60.313,60.313) Tagish Lake ENVELOPE(-134.233,-134.233,59.717,59.717) The Astrophysical Journal 736 1 23
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic meteors
meteorites
meteoroids
nucleosynthesis
abundances
nuclear reactions
supernovae: general
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry
spellingShingle meteors
meteorites
meteoroids
nucleosynthesis
abundances
nuclear reactions
supernovae: general
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry
Petitat, M.
Birck, J.-L.
Luu, T., H
Gounelle, M.
THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE
topic_facet meteors
meteorites
meteoroids
nucleosynthesis
abundances
nuclear reactions
supernovae: general
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry
description thesis of Manuel Petitat at the Laboratoire de Minéralogie et de Cosmochimie du Muséum National d’Histoire Naturelle, Paris and was supported by the Origin network (Marie Curie European Fellowship) International audience Early solar materials bear a variety of isotopic anomalies that reflect compositional differences deriving from distinct stellar nucleosynthetic processes. As shown in previous studies, the stepwise dissolution with increasing acid strengths of bulk rock carbonaceous chondrites liberates Cr with both excesses and deficits in 53 Cr and 54 Cr relative to the terrestrial standard. The magnitude of the 54 Cr variations within a meteorite decreases in the sequence CI1 > CR2 > CM2 > CV3 > CO3 > CK4 and correlates with the degree of metamorphism of each carbonaceous chondrite class. This study shows that the Tagish Lake meteorite presents the highest excesses in 54 Cr ever measured in a bulk silicate phase. According to this study, the Tagish Lake meteorite is composed of the least re-equilibrated material known at this time. The magnitude of 54 Cr variation decreases now in the following sequence: Tagish Lake (ungrouped CI2) > Orgueil (CI1) > Murchison (CM2) > Allende (CV2). Moreover, this study shows that excesses in 53 Cr relative to Earth can be interpreted as representing the extent of aqueous alteration on meteorite parent bodies. Finally, the high 54 Cr anomalies measured in this meteorite make Tagish Lake one of the major targets to decipher the host of these anomalies.
author2 Laboratoire de Minéralogie et Cosmochimie du Muséum (LMCM)
Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS)
Institut de Physique du Globe de Paris (IPGP)
Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)
Centre de Recherches Pétrographiques et Géochimiques (CRPG)
Institut national des sciences de l'Univers (INSU - CNRS)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Petitat, M.
Birck, J.-L.
Luu, T., H
Gounelle, M.
author_facet Petitat, M.
Birck, J.-L.
Luu, T., H
Gounelle, M.
author_sort Petitat, M.
title THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE
title_short THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE
title_full THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE
title_fullStr THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE
title_full_unstemmed THE CHROMIUM ISOTOPIC COMPOSITION OF THE UNGROUPED CARBONACEOUS CHONDRITE TAGISH LAKE
title_sort chromium isotopic composition of the ungrouped carbonaceous chondrite tagish lake
publisher HAL CCSD
publishDate 2011
url https://insu.hal.science/insu-02163323
https://insu.hal.science/insu-02163323/document
https://insu.hal.science/insu-02163323/file/Petitat_2011_ApJ_736_23.pdf
https://doi.org/10.1088/0004-637X/736/1/23
long_lat ENVELOPE(144.250,144.250,-67.317,-67.317)
ENVELOPE(-134.272,-134.272,60.313,60.313)
ENVELOPE(-134.233,-134.233,59.717,59.717)
geographic Murchison
Tagish
Tagish Lake
geographic_facet Murchison
Tagish
Tagish Lake
genre Tagish
genre_facet Tagish
op_source ISSN: 0004-637X
EISSN: 1538-4357
The Astrophysical Journal
https://insu.hal.science/insu-02163323
The Astrophysical Journal, 2011, 736 (1), pp.23. ⟨10.1088/0004-637X/736/1/23⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/736/1/23
insu-02163323
https://insu.hal.science/insu-02163323
https://insu.hal.science/insu-02163323/document
https://insu.hal.science/insu-02163323/file/Petitat_2011_ApJ_736_23.pdf
doi:10.1088/0004-637X/736/1/23
op_rights info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1088/0004-637X/736/1/23
container_title The Astrophysical Journal
container_volume 736
container_issue 1
container_start_page 23
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