Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir

International audience Introduction: Secondary phases in hydrated Antarctic micrometeorites (AMMs) will show an oxygen isotopic signature from their likely formation by aque-ous processes, in either a comet or asteroid parent body. Asteroidal water may be distinguishable from cometary water in its o...

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Main Authors: Dobrica, Elena, Ogliore, R, Engrand, Cecile, Nagashima, K, Brearley, A. J.
Other Authors: Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Format: Conference Object
Language:English
Published: HAL CCSD 2018
Subjects:
Online Access:https://hal.science/hal-02360861
https://hal.science/hal-02360861/document
https://hal.science/hal-02360861/file/Dobrica_2018_MMs_Oiso_hydrated_Mt-LPSC.pdf
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spelling ftccsdartic:oai:HAL:hal-02360861v1 2023-06-18T03:36:22+02:00 Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir Dobrica, Elena Ogliore, R, Engrand, Cecile Nagashima, K Brearley, A. J. Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM) Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Houston, United States 2018-03-19 https://hal.science/hal-02360861 https://hal.science/hal-02360861/document https://hal.science/hal-02360861/file/Dobrica_2018_MMs_Oiso_hydrated_Mt-LPSC.pdf en eng HAL CCSD hal-02360861 https://hal.science/hal-02360861 https://hal.science/hal-02360861/document https://hal.science/hal-02360861/file/Dobrica_2018_MMs_Oiso_hydrated_Mt-LPSC.pdf info:eu-repo/semantics/OpenAccess Lunar Planet. Sci. Lunar and Planetary Science Conference https://hal.science/hal-02360861 Lunar and Planetary Science Conference, Mar 2018, Houston, United States. pp.2666 [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/conferenceObject Conference papers 2018 ftccsdartic 2023-06-04T04:28:00Z International audience Introduction: Secondary phases in hydrated Antarctic micrometeorites (AMMs) will show an oxygen isotopic signature from their likely formation by aque-ous processes, in either a comet or asteroid parent body. Asteroidal water may be distinguishable from cometary water in its oxygen isotopic composition. The oxygen isotopic composition of water in asteroi-dal-derived hydrated AMMs should be close to Δ 17 O ~ 0 if their parent body is carbonaceous chondrite (CC)-like (similar to the hydrated interplanetary dust particles (IDPs) measured so far [1]) or Δ 17 O ~ +6.6‰ if their parent body is ordinary chondrite (OC)-like [e.g. 2-4]. Any hydrated AMMs with significantly different Δ 17 O values would be evidence that these particles formed from non-asteroidal water. If Jupiter-family comets (JFCs) accreted outer nebular water, the O composition of their secondary minerals could be similar to the cosmic symplectites (COSs) from Acfer 094 [5-6]. Here we present the mineralogy and oxygen isotope compositions of magnetite grains and a magnetite-dolomite assemblage that were identified in five AMMs. The purpose of these measurements is to investigate the diversity of the water reservoir from which hydrated AMMs formed and the temperature at which these minerals co-precipitated. Conference Object Antarc* Antarctic Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Antarctic Jupiter ENVELOPE(101.133,101.133,-66.117,-66.117)
institution Open Polar
collection Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe)
op_collection_id ftccsdartic
language English
topic [SDU]Sciences of the Universe [physics]
spellingShingle [SDU]Sciences of the Universe [physics]
Dobrica, Elena
Ogliore, R,
Engrand, Cecile
Nagashima, K
Brearley, A. J.
Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir
topic_facet [SDU]Sciences of the Universe [physics]
description International audience Introduction: Secondary phases in hydrated Antarctic micrometeorites (AMMs) will show an oxygen isotopic signature from their likely formation by aque-ous processes, in either a comet or asteroid parent body. Asteroidal water may be distinguishable from cometary water in its oxygen isotopic composition. The oxygen isotopic composition of water in asteroi-dal-derived hydrated AMMs should be close to Δ 17 O ~ 0 if their parent body is carbonaceous chondrite (CC)-like (similar to the hydrated interplanetary dust particles (IDPs) measured so far [1]) or Δ 17 O ~ +6.6‰ if their parent body is ordinary chondrite (OC)-like [e.g. 2-4]. Any hydrated AMMs with significantly different Δ 17 O values would be evidence that these particles formed from non-asteroidal water. If Jupiter-family comets (JFCs) accreted outer nebular water, the O composition of their secondary minerals could be similar to the cosmic symplectites (COSs) from Acfer 094 [5-6]. Here we present the mineralogy and oxygen isotope compositions of magnetite grains and a magnetite-dolomite assemblage that were identified in five AMMs. The purpose of these measurements is to investigate the diversity of the water reservoir from which hydrated AMMs formed and the temperature at which these minerals co-precipitated.
author2 Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
format Conference Object
author Dobrica, Elena
Ogliore, R,
Engrand, Cecile
Nagashima, K
Brearley, A. J.
author_facet Dobrica, Elena
Ogliore, R,
Engrand, Cecile
Nagashima, K
Brearley, A. J.
author_sort Dobrica, Elena
title Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir
title_short Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir
title_full Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir
title_fullStr Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir
title_full_unstemmed Oxygen isotope systematics of magnetite in hydrated Antarctic micrometeorites: new water reservoir
title_sort oxygen isotope systematics of magnetite in hydrated antarctic micrometeorites: new water reservoir
publisher HAL CCSD
publishDate 2018
url https://hal.science/hal-02360861
https://hal.science/hal-02360861/document
https://hal.science/hal-02360861/file/Dobrica_2018_MMs_Oiso_hydrated_Mt-LPSC.pdf
op_coverage Houston, United States
long_lat ENVELOPE(101.133,101.133,-66.117,-66.117)
geographic Antarctic
Jupiter
geographic_facet Antarctic
Jupiter
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source Lunar Planet. Sci.
Lunar and Planetary Science Conference
https://hal.science/hal-02360861
Lunar and Planetary Science Conference, Mar 2018, Houston, United States. pp.2666
op_relation hal-02360861
https://hal.science/hal-02360861
https://hal.science/hal-02360861/document
https://hal.science/hal-02360861/file/Dobrica_2018_MMs_Oiso_hydrated_Mt-LPSC.pdf
op_rights info:eu-repo/semantics/OpenAccess
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