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

Authors :
Beatrice Pelorosso
Costanza Bonadiman
Michel Grégoire
Theodoros Ntaflos
Alberto Zanetti
Silvia Gentili
Massimo Coltorti
Dipartimento di Fisica e Scienze della Terra [Ferrara]
Università degli Studi di Ferrara (UniFE)
Department of Lithospheric Research [Wien]
Universität Wien
Géosciences Environnement Toulouse (GET)
Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP)
Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)
Dipartimento di Fisica e Geologia [Perugia]
Università degli Studi di Perugia (UNIPG)
Instituto di Geoscienze e Georisorse
Consiglio Nazionale delle Ricerche (CNR)
Università degli Studi di Ferrara = University of Ferrara (UniFE)
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)
Università degli Studi di Perugia = University of Perugia (UNIPG)
National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR)
Source :
Contributions to Mineralogy and Petrology, Contributions to Mineralogy and Petrology, Springer Verlag, 2019, 174 (5), ⟨10.1007/s00410-019-1579-1⟩, Contributions to Mineralogy and Petrology, 2019, 174 (5), ⟨10.1007/s00410-019-1579-1⟩, Contributions to mineralogy and petrology 174 (2019). doi:10.1007/s00410-019-1579-1, info:cnr-pdr/source/autori:Pelorosso B.[1], Bonadiman C.[1], Ntaflos T.[2], Gregoire M.[3], Gentili S.[4], Zanetti A.[5], Coltorti M.[1]/titolo:An insight into the first stages of the Ferrar magmatism: ultramafic cumulates from Harrow Peaks, northern Victoria Land, Antarctica/doi:10.1007%2Fs00410-019-1579-1/rivista:Contributions to mineralogy and petrology/anno:2019/pagina_da:/pagina_a:/intervallo_pagine:/volume:174
Publication Year :
2019
Publisher :
Springer Science and Business Media LLC, 2019.

Abstract

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.

Details

ISSN :
14320967 and 00107999
Volume :
174
Database :
OpenAIRE
Journal :
Contributions to Mineralogy and Petrology
Accession number :
edsair.doi.dedup.....faf87b99bb58f29f0913484e14361a68
Full Text :
https://doi.org/10.1007/s00410-019-1579-1