Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9588
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dc.contributor.authorallGaeta, M.; università La Sapienza Romaen
dc.contributor.authorallGiuliani, A.; School of Earth Sciences Australiaen
dc.contributor.authorallPerilla, S.; Università La Sapienza Romaen
dc.contributor.authorallMisiti, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.date.accessioned2015-05-13T10:10:39Zen
dc.date.available2015-05-13T10:10:39Zen
dc.date.issued2013en
dc.identifier.urihttp://hdl.handle.net/2122/9588en
dc.description.abstractThe mineralogy of thermometamorphic granites is relatively simple, making it possible to track the spatial distribution of chemical and mineralogical variations in these rocks and investigate the processes that underpin these metamorphic reactions.We have undertaken a detailed investigation of metagranites from the contact aureole that fringes a quartz diorite intrusion of Late Permian age, emplaced into Carboniferous peraluminous granites of the Gennargentu Igneous Complex (Sardinia, Italy). New data are presented including the petrography of metagranites within a 500 m zone adjacent to the quartz diorite intrusion, the compositions of minerals and bulk-rocks, and the oxygen isotope compositions of separated minerals. We have used these data to assess the mobility of elements, expressed as oxide, in the aureole, and the physical conditions of fluid-assisted thermometamorphism. Modal variations and the oscillatory zoning of plagioclase demonstrate that the shallow (P 200MPa) quartz diorite intrusion was emplaced through a number of magmatic injections.The border zone of the quartz diorite intrusion presents evidence of two main processes: hybridization between andesite and rhyolite magmas and volatile saturation of the mingled magma. Modal differences in the contact zone with respect to the protolith (i.e. peraluminous granite), variations in mineral composition, temperature constraints and K2O, Na2O, SiO2 and Al2O3 indicate that a relatively large volume of the host granite (up to 400 m from the contact) was metasomatized by high-temperature (650^3508C) fluids derived from the mingled zone of the quartz diorite intrusion. In detail, the metasomatic K2O-rich fluid reacted with albite to form K-feldspar, and triggered the recrystallization of quartz and plagioclase to higher calcium concentrations. The progressive increase in the MgO/(MgOþFeO) of chlorite closer to the contact indicates that this phase also recrystallized. The iron released during chlorite recrystallization was buffered by hematite formation in the pores of metasomatic K-feldspar. The Gennargentu metagranites provide evidence that metasomatic fluids can play a major role in driving metamorphic reactions in contact aureoles. For instance, the expected increase of Ca in plagioclase owing to thermal equilibration was not achieved in the high-T zone of the aureole because of fluid-assisted removal of cations.We conclude that caution should be taken when interpreting the processes that underpin contact metamorphism in terms of thermally driven, ionic diffusion alone, because the role of fluids may be significant, if not overwhelming, in the domains closest to the magmatic source.en
dc.language.isoEnglishen
dc.publisher.nameOxford University Pressen
dc.relation.ispartofJournal of petrologyen
dc.relation.ispartofseries5/54 (2013)en
dc.subjectcontact metamorphismen
dc.subjectmetasomatismen
dc.subjectred metagranitesen
dc.subjectoxygen isotopesen
dc.subjectGennargentu Igneous Complexen
dc.titleReddish Metagranites from the Gennargentu Igneous Complex (Sardinia, Italy): insight into metasomatism induced by magma minglingen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber839-859en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.05. Mineralogy and petrologyen
dc.identifier.doi10.1093/petrology/egs008en
dc.description.obiettivoSpecifico3V. Dinamiche e scenari eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0022-3530en
dc.relation.eissn1460-2415en
dc.contributor.authorGaeta, M.en
dc.contributor.authorGiuliani, A.en
dc.contributor.authorPerilla, S.en
dc.contributor.authorMisiti, V.en
dc.contributor.departmentuniversità La Sapienza Romaen
dc.contributor.departmentSchool of Earth Sciences Australiaen
dc.contributor.departmentUniversità La Sapienza Romaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptUniversità La Sapienza-
crisitem.author.deptSchool of Earth Sciences Australia-
crisitem.author.deptUniversità La Sapienza Roma-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0002-6151-7789-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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