Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/13634
DC FieldValueLanguage
dc.date.accessioned2020-06-24T06:59:00Z-
dc.date.available2020-06-24T06:59:00Z-
dc.date.issued2020-06-
dc.identifier.urihttp://hdl.handle.net/2122/13634-
dc.description.abstractLascar (5592 m a.s.l.) and Lastarria (5697 m a.s.l.) are Chilean active stratovolcanoes located in the Central Volcanic Zone (CVZ; 16°S to 28°S) that have developed on top of a 71 km thick continental crust. Independently of the similarities in their Plinian/Vulcanian eruptive styles, their complex magmatic feeding structures and the origins of their magmatic fluids still necessitate constraints in order to improve the reliability of geochemical monitoring. Here we investigate the petrography, bulk-rock chemistry, and mineral chemistry in products from the 1986–1993 explosive eruptive cycle at Lascar and from several Holocene eruptive sequences at Lastarria. These data are integratedwith measurements of the noble gas isotopes in fluid inclusions (FIs) of minerals fromthe same products as well as in fumarole gases. The geochemistry ofminerals and rocks shows that the studied products belong to high-K–calc-alkaline series typical of subduction-related settings, and provide evidence of differentiation,mixing, and crustal assimilation that are higher at Lastarria. The contribution of slab sediments and fluids to magma genesis in thewedge is limited, suggesting a homogeneous mantle beneath CVZ. The deepest crystallization processes occurred at variable levels of the plumbing systems according to the lithostatic equivalent depths estimated with mineral equilibrium geobarometers at Lascar (15–29 km) and Lastarria (~20–40 km). The 40Ar/36Ar and 4He/20Ne ratios in FIs and fumarole gases indicate the presence of some degree of air contamination in the fluids from both volcanoes. The 3He/4He values at Lascar (6.9–7.3 Ra) are relatively homogeneous and comparable to those of fumaroles, suggesting a main zone of magma crystallization and degassing. In contrast, the 3He/4He values at Lastarria (5.31–8.01 Ra) vary over a wide range, suggesting various magma storage levels and providing evidence of crustal contamination, as indicated by the rock chemistry.We argue thatmantle beneath the two volcanoes has a MORB-like signature of 3He/4He, while local crustal contamination explains the lower ratios measured at Lascar.en_US
dc.language.isoEnglishen_US
dc.publisher.nameElsevieren_US
dc.relation.ispartofLithosen_US
dc.relation.ispartofseries/370-371 (2020)en_US
dc.subjectLascaren_US
dc.subjectLastarriaen_US
dc.subjectnoble gasesen_US
dc.subjectFluid inclusionsen_US
dc.subjectCrustal contaminationen_US
dc.subjectMantle wedgeen_US
dc.titlePetrological and noble gas features of Lascar and Lastarria volcanoes (Chile): Inferences on plumbing systems and mantle characteristicsen_US
dc.typearticleen
dc.description.statusPublisheden_US
dc.type.QualityControlPeer-revieweden_US
dc.description.pagenumber105615en_US
dc.subject.INGV04.08. Volcanologyen_US
dc.subject.INGV04.01. Earth Interioren_US
dc.identifier.doi10.1016/j.lithos.2020.105615en_US
dc.description.obiettivoSpecifico1V. Storia eruttivaen_US
dc.description.obiettivoSpecifico2V. Struttura e sistema di alimentazione dei vulcanien_US
dc.description.journalTypeJCR Journalen_US
dc.relation.issn0024-4937en_US
dc.contributor.authorRobidoux, Philippe-
dc.contributor.authorRizzo, Andrea Luca-
dc.contributor.authorAguilera, Felipe-
dc.contributor.authorAiuppa, Alessandro-
dc.contributor.authorArtale, Maria-
dc.contributor.authorLiuzzo, Marco-
dc.contributor.authorNazzari, Manuela-
dc.contributor.authorZummo, Francesco Paolo-
dc.contributor.departmentUniversidad de Chileen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italiaen_US
dc.contributor.departmentUniversidad Católica del Norteen_US
dc.contributor.departmentUniversità di Palermoen_US
dc.contributor.departmentUniversità di Palermoen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italiaen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen_US
dc.contributor.departmentUniversità di Palermoen_US
item.cerifentitytypePublications-
item.fulltextWith Fulltext-
item.languageiso639-1en-
item.openairetypearticle-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptUniversità di Palermo-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptUniversità di Palermo-
crisitem.author.orcid0000-0002-6099-5295-
crisitem.author.orcid0000-0003-2225-3781-
crisitem.author.orcid0000-0002-0254-6539-
crisitem.author.orcid0000-0001-5566-1568-
crisitem.author.orcid0000-0002-3099-7505-
crisitem.author.orcid0000-0001-5926-5773-
crisitem.author.orcid0000-0001-5923-1784-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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