Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures

International audience Most kimberlites contain abundant dunitic nodules. These are centimetre-sized, rounded and multi-grained assemblages of xenocrystic olivine with a wide range of compositions (Fo83 to Fo94). The absence of orthopyroxene and other mantle minerals and the range of olivine composi...

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Published in:Journal of Petrology
Main Authors: Cordier, Carole, Sauzeat, Lucie, Arndt, Nicholas T., Boullier, Anne-Marie, Batanova, Valentina, Barou, Fabrice
Other Authors: Institut des Sciences de la Terre (ISTerre), Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Géosciences Montpellier, Institut national des sciences de l'Univers (INSU - CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université des Antilles (UA)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2015
Subjects:
Online Access:https://hal.science/hal-01277963
https://doi.org/10.1093/petrology/egv054
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spelling ftunivantilles:oai:HAL:hal-01277963v1 2024-04-28T08:22:27+00:00 Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures Cordier, Carole Sauzeat, Lucie Arndt, Nicholas T. Boullier, Anne-Marie Batanova, Valentina Barou, Fabrice Institut des Sciences de la Terre (ISTerre) Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS) Géosciences Montpellier Institut national des sciences de l'Univers (INSU - CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université des Antilles (UA) 2015-09 https://hal.science/hal-01277963 https://doi.org/10.1093/petrology/egv054 en eng HAL CCSD Oxford University Press (OUP) info:eu-repo/semantics/altIdentifier/doi/10.1093/petrology/egv054 hal-01277963 https://hal.science/hal-01277963 doi:10.1093/petrology/egv054 ISSN: 0022-3530 EISSN: 1460-2415 Journal of Petrology https://hal.science/hal-01277963 Journal of Petrology, 2015, 56 (9), pp.1775-1795. ⟨10.1093/petrology/egv054⟩ dunite grain boundary migration kimberlite metasomatism olivine xenocryst [SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography info:eu-repo/semantics/article Journal articles 2015 ftunivantilles https://doi.org/10.1093/petrology/egv054 2024-04-10T23:56:38Z International audience Most kimberlites contain abundant dunitic nodules. These are centimetre-sized, rounded and multi-grained assemblages of xenocrystic olivine with a wide range of compositions (Fo83 to Fo94). The absence of orthopyroxene and other mantle minerals and the range of olivine compositions have been attributed to reaction between mantle peridotite and (proto)kimberlitic fluid or melt, but the timing of the reaction is a subject of debate. In a kimberlite from the Kangamiut region of Greenland, nodule cores are surrounded by fine-grained outer margins with near-constant Fo contents (∼Fo88) but highly variable minor element contents (e.g. 500–2500 ppm Ni). These margins crystallized from the kimberlite melt and we show that their compositions can be explained by crystallization of olivine alone, if a high partition coefficient for Ni between melt and olivine (DNi > 20) is assumed. Orthopyroxene assimilation is not required, removing the constraint that its dissolution occurred during ascent of the kimberlite magma. Within some nodules, in addition to the usual core-to-margin gradients, we observe asymmetric compositional changes (variable Fo but near-constant minor element contents) across mobile grain boundaries. These changes document fluid percolation at the grain scale that occurred during dynamic recrystallization in the deforming lithospheric mantle. We note that chemical gradients associated with mobile grain boundaries are observed in olivines that cover the entire compositional range of the nodules, and propose that fluid-assisted dynamic recrystallization took place in dunite that was already compositionally heterogeneous. Reaction between peridotite and protokimberlitic melt or fluid and dissolution of orthopyroxene thus occurred within the lithospheric mantle, immediately (a few days) prior to the ascent of the kimberlite melt and the entrainment of the dunite nodules. We propose that the grain boundary zones probably mimic, at a fine scale, the fluid–peridotite interaction that ... Article in Journal/Newspaper Greenland Université des Antilles (UAG): HAL Journal of Petrology 56 9 1775 1796
institution Open Polar
collection Université des Antilles (UAG): HAL
op_collection_id ftunivantilles
language English
topic dunite
grain boundary migration
kimberlite
metasomatism
olivine xenocryst
[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography
spellingShingle dunite
grain boundary migration
kimberlite
metasomatism
olivine xenocryst
[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography
Cordier, Carole
Sauzeat, Lucie
Arndt, Nicholas T.
Boullier, Anne-Marie
Batanova, Valentina
Barou, Fabrice
Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures
topic_facet dunite
grain boundary migration
kimberlite
metasomatism
olivine xenocryst
[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography
description International audience Most kimberlites contain abundant dunitic nodules. These are centimetre-sized, rounded and multi-grained assemblages of xenocrystic olivine with a wide range of compositions (Fo83 to Fo94). The absence of orthopyroxene and other mantle minerals and the range of olivine compositions have been attributed to reaction between mantle peridotite and (proto)kimberlitic fluid or melt, but the timing of the reaction is a subject of debate. In a kimberlite from the Kangamiut region of Greenland, nodule cores are surrounded by fine-grained outer margins with near-constant Fo contents (∼Fo88) but highly variable minor element contents (e.g. 500–2500 ppm Ni). These margins crystallized from the kimberlite melt and we show that their compositions can be explained by crystallization of olivine alone, if a high partition coefficient for Ni between melt and olivine (DNi > 20) is assumed. Orthopyroxene assimilation is not required, removing the constraint that its dissolution occurred during ascent of the kimberlite magma. Within some nodules, in addition to the usual core-to-margin gradients, we observe asymmetric compositional changes (variable Fo but near-constant minor element contents) across mobile grain boundaries. These changes document fluid percolation at the grain scale that occurred during dynamic recrystallization in the deforming lithospheric mantle. We note that chemical gradients associated with mobile grain boundaries are observed in olivines that cover the entire compositional range of the nodules, and propose that fluid-assisted dynamic recrystallization took place in dunite that was already compositionally heterogeneous. Reaction between peridotite and protokimberlitic melt or fluid and dissolution of orthopyroxene thus occurred within the lithospheric mantle, immediately (a few days) prior to the ascent of the kimberlite melt and the entrainment of the dunite nodules. We propose that the grain boundary zones probably mimic, at a fine scale, the fluid–peridotite interaction that ...
author2 Institut des Sciences de la Terre (ISTerre)
Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)
Géosciences Montpellier
Institut national des sciences de l'Univers (INSU - CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université des Antilles (UA)
format Article in Journal/Newspaper
author Cordier, Carole
Sauzeat, Lucie
Arndt, Nicholas T.
Boullier, Anne-Marie
Batanova, Valentina
Barou, Fabrice
author_facet Cordier, Carole
Sauzeat, Lucie
Arndt, Nicholas T.
Boullier, Anne-Marie
Batanova, Valentina
Barou, Fabrice
author_sort Cordier, Carole
title Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures
title_short Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures
title_full Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures
title_fullStr Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures
title_full_unstemmed Metasomatism of the Lithospheric Mantle Immediately Precedes Kimberlite Eruption: New Evidence from Olivine Composition and Microstructures
title_sort metasomatism of the lithospheric mantle immediately precedes kimberlite eruption: new evidence from olivine composition and microstructures
publisher HAL CCSD
publishDate 2015
url https://hal.science/hal-01277963
https://doi.org/10.1093/petrology/egv054
genre Greenland
genre_facet Greenland
op_source ISSN: 0022-3530
EISSN: 1460-2415
Journal of Petrology
https://hal.science/hal-01277963
Journal of Petrology, 2015, 56 (9), pp.1775-1795. ⟨10.1093/petrology/egv054⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1093/petrology/egv054
hal-01277963
https://hal.science/hal-01277963
doi:10.1093/petrology/egv054
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container_title Journal of Petrology
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