Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9253
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dc.contributor.authorallMisiti, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallVetere, F.; Università degli Studi di Perugiaen
dc.contributor.authorallHeidelbach, F.; Bayerisches Geoinstituten
dc.date.accessioned2015-01-15T09:41:06Zen
dc.date.available2015-01-15T09:41:06Zen
dc.date.issued2014en
dc.identifier.urihttp://hdl.handle.net/2122/9253en
dc.description.abstractPlagioclase crystal size distribution (CSD) has been investigated in a quartz-diorite body, in the leucosome of migmatites and in the melanosome of un-melted contact metamorphic rocks from Gennargentu Complex (Sardinia, Italy). During the crystallization of the dioritic magma, a variety of competing kinetic processes determine the evolution of the igneous microstructure, but the relative contribution of each process remains elusive. Our approach was aimed to study the plagioclase crystallization from a liquid (quartz-diorites and migmatite leucosomes), comparing it to a crystallization at subsolidus conditions. CSD indicates that plagioclase in the quartz-diorite nucleated and grew in a cooling system at a constant cooling rate, producing straight-line CSD in a diagram of ln of population density vs. size range. The plagioclase crystallization continued until the latent heat was available and the temperature was high enough to allow the plagioclase growing. This can occur only when a crystal is held at temperature close to its liquidus for a long period of time. Under these conditions, the plagioclase nucleation rate is zero, but growth rate is high for crystal larger than the critical size. This does not necessarily mean that the temperature was held constant, just that the undercooling remained small (Ostwald ripening process). The aggregated small crystals, due to their high surface energy per unit volume, to minimise energy in the system dissolved and“fed” the growth of larger crystals. This process occurs because small grains have a higher surface energy per unit volume than do larger grains. The crystallization temperature (~900 °C, 100 MPa) allows the formation of plagioclase as liquidus phase. From CSD measurements we calculated the different cooling ages for the different sample typesen
dc.language.isoEnglishen
dc.relation.ispartofPeriofico di Mineralogiaen
dc.relation.ispartofseries/83 (2014)en
dc.subjectcrystal size distributionen
dc.subjectGennargentu Igneous Complexen
dc.subjectplagioclaseen
dc.subjectsubsolidus crystallisationen
dc.subjectOstwald ripeningen
dc.titleCrystallization from a melt and crystallization at subsolidus conditions: comparison from crystal size distribution study on Gennargentu Rocks (Sardinia, Italy)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber401-418en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.05. Mineralogy and petrologyen
dc.identifier.doi10.2451/2014PM0022en
dc.description.obiettivoSpecifico4V. Vulcani e ambienteen
dc.description.journalTypeN/A or not JCRen
dc.description.fulltextrestricteden
dc.contributor.authorMisiti, V.en
dc.contributor.authorVetere, F.en
dc.contributor.authorHeidelbach, F.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentUniversità degli Studi di Perugiaen
dc.contributor.departmentBayerisches Geoinstituten
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptBayerisches Geoinstitut-
crisitem.author.orcid0000-0002-6151-7789-
crisitem.author.orcid0000-0002-0723-1990-
crisitem.author.orcid0000-0001-8838-2311-
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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