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<title lang=en>Spatial variability of pyroxenite layers in the Beni Bousera orogenic peridotite (Morocco) and implications for their origin</title>
<creator>Chetouani, Kamar</creator>
<creator>BODINIER, Jean-louis</creator>
<creator>Garrido, C. J.</creator>
<creator>Marchesi, Claudio</creator>
<creator>Amri, Isma</creator>
<creator>Targuisti, Kamal</creator>
<contributor>Université Abdelmalek Essaâdi</contributor>
<contributor>Géosciences Montpellier ; Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Manteau et Interfaces ; Géosciences Montpellier ; Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS) - Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Instituto Andaluz de Ciencias de la Tierra (IACT) ; Universidad de Granada (UGR) - Consejo Superior de Investigaciones Científicas [Spain] (CSIC)</contributor>
<contributor>MAE (France), MESRSFC (Morocco), and CNRS/INSU (France) through the cooperation project #042/STU/09 in the frame of the ‘Volubilis Hubert Curien’ program (2010–2013) and three INSU research grants (‘Actions coordonne´ es’ 2008, and SYSTER 2010 and 2011).</contributor>
<source>ISSN: 1631-0713</source>
<source>Comptes Rendus Géoscience</source>
<publisher>Elsevier Masson</publisher>
<identifier>hal-01468018</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-01468018</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-01468018/document</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-01468018/file/chetouani.pdf</identifier>
<source>https://hal.archives-ouvertes.fr/hal-01468018</source>
<source>Comptes Rendus Géoscience, Elsevier Masson, 2016, 348 (8), pp.619-629. 〈10.1016/j.crte.2016.06.001〉</source>
<identifier>DOI : 10.1016/j.crte.2016.06.001</identifier>
<relation>info:eu-repo/semantics/altIdentifier/doi/10.1016/j.crte.2016.06.001</relation>
<language>en</language>
<subject lang=en>Crustal recycling</subject>
<subject lang=en>Melt-rock reaction</subject>
<subject lang=en>Mantle pyroxenite</subject>
<subject lang=en>Orogenic peridotite</subject>
<subject lang=en>Beni Bousera</subject>
<subject>[SDU.STU.PE] Sciences of the Universe [physics]/Earth Sciences/Petrography</subject>
<type>info:eu-repo/semantics/article</type>
<type>Journal articles</type>
<description lang=en>The Beni Bousera peridotite contains a diversity of pyroxenite layers. Several studies have postulated that at least some of them represent elongated strips of oceanic lithosphere recycled in the convective mantle. Some pyroxenites were, however, ascribed to igneous crystal segregation or melt–rock reactions. To further constrain the origin of these rocks, we collected 171 samples throughout the massif and examined their variability in relation with the tectono-metamorphic domains. A major finding is that all facies showing clear evidence for a crustal origin are concentrated in a narrow corridor of mylonitized peridotites, along the contact with granulitic country rocks. These peculiar facies were most likely incorporated at the mantle–crust boundary during the orogenic events that culminated in the peridotite exhumation. The other pyroxenites derive from a distinct protolith that was ubiquitous in the massif before its exhumation. They were deeply modified by partial melting and melt–rock reactions associated with lithospheric thinning.</description>
<date>2016</date>
<contributor>European Project : 612572, EC:FP7:PEOPLE, FP7-PEOPLE-2013-IRSES, MEDYNA(2014)</contributor>
<relation>info:eu-repo/grantAgreement/EC/FP7/612572/EU/MAGHREB-EU RESEARCH STAFF EXCHANGE ON GEODYNAMICS, GEOHZARDS, AND APPLIED GEOLOGY IN NORTH-WEST AFRICA/MEDYNA</relation>
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