An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica

International audience A group of ultramafic xenoliths hosted in Cenozoic hypabyssal rocks from Harrow Peaks (northern Victoria Land, Antarctica) show textural and geochemical features far removed from anything previously observed in mantle xenoliths of this region and elsewhere in Antarctica. They...

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Published in:Contributions to Mineralogy and Petrology
Main Authors: Pelorosso, Beatrice, Bonadiman, Costanza, Ntaflos, Theodoros, Gregoire, Michel, Gentili, Silvia, Zanetti, Alberto, Coltorti, Massimo
Other Authors: Dipartimento di Fisica e Scienze della Terra Ferrara, Università degli Studi di Ferrara = University of Ferrara (UniFE), Department of Lithospheric Research Wien, Universität Wien, Géosciences Environnement Toulouse (GET), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS), Dipartimento di Fisica e Geologia Perugia, Università degli Studi di Perugia = University of Perugia (UNIPG), Instituto di Geoscienze e Georisorse, National Research Council of Italy
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2019
Subjects:
Online Access:https://hal.science/hal-02363207
https://hal.science/hal-02363207/document
https://hal.science/hal-02363207/file/Pelorosso%20et%20al_2019.pdf
https://doi.org/10.1007/s00410-019-1579-1
id ftutoulouse3hal:oai:HAL:hal-02363207v1
record_format openpolar
institution Open Polar
collection Université Toulouse III - Paul Sabatier: HAL-UPS
op_collection_id ftutoulouse3hal
language English
topic ultramafic xenoliths
high-Mg magmatic olivines
orthopyroxenite
Karoo-Ferrar large igneous province
[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography
[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry
[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
spellingShingle ultramafic xenoliths
high-Mg magmatic olivines
orthopyroxenite
Karoo-Ferrar large igneous province
[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography
[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry
[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
Pelorosso, Beatrice
Bonadiman, Costanza
Ntaflos, Theodoros
Gregoire, Michel
Gentili, Silvia
Zanetti, Alberto
Coltorti, Massimo
An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica
topic_facet ultramafic xenoliths
high-Mg magmatic olivines
orthopyroxenite
Karoo-Ferrar large igneous province
[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography
[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry
[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
description International audience A group of ultramafic xenoliths hosted in Cenozoic hypabyssal rocks from Harrow Peaks (northern Victoria Land, Antarctica) show textural and geochemical features far removed from anything previously observed in mantle xenoliths of this region and elsewhere in Antarctica. They consist of spinel-bearing lherzolites and harzburgites, characterised by a predominant equigranular texture with orthopyroxene modal contents remarkably higher in lherzolites (18-26 volume%) with respect to the harzburgite (13 vol%), one orthopyroxenite, and three composite xenoliths. The latter are formed by an olivine-dominant assemblage (olivine > 70%) crosscut by large monomineralic (amphibole or clinopyroxene) or bimineralic (amphibole + clino-pyroxene) veins. No significant correlation was observed between the lithology and the Fo content (90.21-82.81) of olivine, suggesting that these rocks could be derived from a cumulus process. The presence of the orthopyroxenite suggests that the inferred melt/s from which they stemmed was close (or even above) to silica saturation. Based on major and trace-element mineral/melt and mineral/mineral equilibrium modelling, these rocks were formed by progressive extraction of olivine from a high magnesium (Mg = 72)-high temperature (~ 1300 °C) melt following a very short fractionation line. Thermobaro-metric results indicate the stationing of Harrow Peaks cumulates in the P field of 1.3 ± 0.2 (dunites)-0.5 ± 0.2 (orthopy-roxenite) GPa. These values well match the crust/mantle boundary (Moho) of the region. The combined geochemical and petrological data suggest that Harrow Peaks melts could be related to the initial stage of the Jurassic Ferrar magmatism, whose deep cumulates were subsequently affected by the Cenozoic alkaline metasomatism, widely detected in the northern Victoria Land lithosphere and responsible for the formation of the late amphibole/amphibole + clinopyroxene veins.
author2 Dipartimento di Fisica e Scienze della Terra Ferrara
Università degli Studi di Ferrara = University of Ferrara (UniFE)
Department of Lithospheric Research Wien
Universität Wien
Géosciences Environnement Toulouse (GET)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)
Dipartimento di Fisica e Geologia Perugia
Università degli Studi di Perugia = University of Perugia (UNIPG)
Instituto di Geoscienze e Georisorse
National Research Council of Italy
format Article in Journal/Newspaper
author Pelorosso, Beatrice
Bonadiman, Costanza
Ntaflos, Theodoros
Gregoire, Michel
Gentili, Silvia
Zanetti, Alberto
Coltorti, Massimo
author_facet Pelorosso, Beatrice
Bonadiman, Costanza
Ntaflos, Theodoros
Gregoire, Michel
Gentili, Silvia
Zanetti, Alberto
Coltorti, Massimo
author_sort Pelorosso, Beatrice
title An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica
title_short An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica
title_full An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica
title_fullStr An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica
title_full_unstemmed An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica
title_sort insight into the first stages of the ferrar magmatism: ultramafic cumulates from harrow peaks, northern victoria land, antarctica
publisher HAL CCSD
publishDate 2019
url https://hal.science/hal-02363207
https://hal.science/hal-02363207/document
https://hal.science/hal-02363207/file/Pelorosso%20et%20al_2019.pdf
https://doi.org/10.1007/s00410-019-1579-1
long_lat ENVELOPE(164.750,164.750,-74.067,-74.067)
geographic Harrow Peaks
Victoria Land
geographic_facet Harrow Peaks
Victoria Land
genre Antarc*
Antarctica
Victoria Land
genre_facet Antarc*
Antarctica
Victoria Land
op_source ISSN: 0010-7999
EISSN: 1432-0967
Contributions to Mineralogy and Petrology
https://hal.science/hal-02363207
Contributions to Mineralogy and Petrology, 2019, 174 (5), ⟨10.1007/s00410-019-1579-1⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1007/s00410-019-1579-1
hal-02363207
https://hal.science/hal-02363207
https://hal.science/hal-02363207/document
https://hal.science/hal-02363207/file/Pelorosso%20et%20al_2019.pdf
doi:10.1007/s00410-019-1579-1
op_rights info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1007/s00410-019-1579-1
container_title Contributions to Mineralogy and Petrology
container_volume 174
container_issue 5
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spelling ftutoulouse3hal:oai:HAL:hal-02363207v1 2023-12-17T10:22:10+01:00 An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica Pelorosso, Beatrice Bonadiman, Costanza Ntaflos, Theodoros Gregoire, Michel Gentili, Silvia Zanetti, Alberto Coltorti, Massimo Dipartimento di Fisica e Scienze della Terra Ferrara Università degli Studi di Ferrara = University of Ferrara (UniFE) Department of Lithospheric Research Wien Universität Wien Géosciences Environnement Toulouse (GET) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) Dipartimento di Fisica e Geologia Perugia Università degli Studi di Perugia = University of Perugia (UNIPG) Instituto di Geoscienze e Georisorse National Research Council of Italy 2019 https://hal.science/hal-02363207 https://hal.science/hal-02363207/document https://hal.science/hal-02363207/file/Pelorosso%20et%20al_2019.pdf https://doi.org/10.1007/s00410-019-1579-1 en eng HAL CCSD Springer Verlag info:eu-repo/semantics/altIdentifier/doi/10.1007/s00410-019-1579-1 hal-02363207 https://hal.science/hal-02363207 https://hal.science/hal-02363207/document https://hal.science/hal-02363207/file/Pelorosso%20et%20al_2019.pdf doi:10.1007/s00410-019-1579-1 info:eu-repo/semantics/OpenAccess ISSN: 0010-7999 EISSN: 1432-0967 Contributions to Mineralogy and Petrology https://hal.science/hal-02363207 Contributions to Mineralogy and Petrology, 2019, 174 (5), ⟨10.1007/s00410-019-1579-1⟩ ultramafic xenoliths high-Mg magmatic olivines orthopyroxenite Karoo-Ferrar large igneous province [SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography [SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry [SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy info:eu-repo/semantics/article Journal articles 2019 ftutoulouse3hal https://doi.org/10.1007/s00410-019-1579-1 2023-11-22T18:05:38Z International audience A group of ultramafic xenoliths hosted in Cenozoic hypabyssal rocks from Harrow Peaks (northern Victoria Land, Antarctica) show textural and geochemical features far removed from anything previously observed in mantle xenoliths of this region and elsewhere in Antarctica. They consist of spinel-bearing lherzolites and harzburgites, characterised by a predominant equigranular texture with orthopyroxene modal contents remarkably higher in lherzolites (18-26 volume%) with respect to the harzburgite (13 vol%), one orthopyroxenite, and three composite xenoliths. The latter are formed by an olivine-dominant assemblage (olivine > 70%) crosscut by large monomineralic (amphibole or clinopyroxene) or bimineralic (amphibole + clino-pyroxene) veins. No significant correlation was observed between the lithology and the Fo content (90.21-82.81) of olivine, suggesting that these rocks could be derived from a cumulus process. The presence of the orthopyroxenite suggests that the inferred melt/s from which they stemmed was close (or even above) to silica saturation. Based on major and trace-element mineral/melt and mineral/mineral equilibrium modelling, these rocks were formed by progressive extraction of olivine from a high magnesium (Mg = 72)-high temperature (~ 1300 °C) melt following a very short fractionation line. Thermobaro-metric results indicate the stationing of Harrow Peaks cumulates in the P field of 1.3 ± 0.2 (dunites)-0.5 ± 0.2 (orthopy-roxenite) GPa. These values well match the crust/mantle boundary (Moho) of the region. The combined geochemical and petrological data suggest that Harrow Peaks melts could be related to the initial stage of the Jurassic Ferrar magmatism, whose deep cumulates were subsequently affected by the Cenozoic alkaline metasomatism, widely detected in the northern Victoria Land lithosphere and responsible for the formation of the late amphibole/amphibole + clinopyroxene veins. Article in Journal/Newspaper Antarc* Antarctica Victoria Land Université Toulouse III - Paul Sabatier: HAL-UPS Harrow Peaks ENVELOPE(164.750,164.750,-74.067,-74.067) Victoria Land Contributions to Mineralogy and Petrology 174 5