Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/2970
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dc.contributor.authorallDi Renzo, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallDi Vito, M. A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallArienzo, I.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallCarandente, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallCivetta, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallD'Antonio, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallGiordano, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallOrsi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallTonarini, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.date.accessioned2007-12-06T08:44:12Zen
dc.date.available2007-12-06T08:44:12Zen
dc.date.issued2007en
dc.identifier.urihttp://hdl.handle.net/2122/2970en
dc.description.abstractA continuous-coring borehole recently drilled at Camaldoli dellaTorre on the southern slopes of Somma^Vesuvius provides constraints on the volcanic and magmatic history of the Vesuvian volcanic area since c. 126 ka BP. The cored sequence includes volcanic units, defined on stratigraphical, sedimentological, petrological and geochemical grounds, emitted from both local and distal vents. Some of these units are of known age, such as one Phlegraean pre-Campanian Ignimbrite, Campanian Ignimbrite (39 ka), Neapolitan Yellow Tuff (14 9ka) and Vesuvian Plinian deposits, which helps to constrain the relative age of the other units.The main rock types encountered are shoshonite, phonotephrite, latite, trachyte and phonolite. The sequence includes, from the base upwards: a thick succession of pyroclastic units emplaced between 126 and 39 ka, most of them attributed to eruptions that occurred in the Phlegraean area; the Campanian Ignimbrite; the products of a local tuff cone formed between 39 ka and the deposition of the products of the earliest activity of the Mt. Somma volcano; the products of the Somma^Vesuvius volcano, which include from the base upwards a thick sequence of lavas, pyroclastic rocks and the products of a local spattercone dated between 3 7ka and AD 79.The data obtained from the study of the borehole show that, before the Campanian Ignimbrite eruption, low-energy explosive volcanism took place in the Vesuvian area, whereas mostly high-energy explosive eruptions characterized the Campi Flegrei activity. In the Vesuvian area, Campanian Ignimbrite deposition was followed by the eruption of a local tuff cone and a long repose time, which predated the formation of the Mt. Somma edifice. Since 18 3 ka (Pomici di Base eruption) the activity of Somma^Vesuvius became mostly explosive with rare lava effusions.The shallowest cored deposits belong to the Camaldoli dellaTorre cone, formed between the Pomici di Avellino and Pomici di Pompei eruptions (3 7 ka^AD 79). Newgeochemical and Sr^Nd^Pb^ B-isotopic data on samples from the drilled core, together with those available from the literature, allow us to further distinguish the volcanic rocks as a function of both their provenance (i.e. Phlegraean or Vesuvian areas) and age, and to identify different magmatic processes acting through time in the Vesuvian mantle source(s) and during magma ascent towards the surface. Isotopically distinct magmas, rising from a mantle source variably contaminated by slab- derived components, stagnated at mid-crustal depths (8^10 km below sea level) where magmas differentiated and were probably contaminated. Contamination occurred either with Hercynian continental crust, mostly during the oldest stages of Vesuvian activity (from 39 to 16 ka), or with Mesozoic limestone, mostly during recent Vesuvian activity. Energy constrained assimilation and fractional crystallization (EC-AFC) modelling results show that contamina- tion with Hercynian crust probably occurred during differentiation from shoshonite to latite. Contamination with limestone, which is not well constrained with the available data, might have occurred only during the transition from shoshonite to tephrite. From the ‘deep’ reservoir, magmas rose towards a series of shallow reservoirs, in which they differentiated further, mixed, and fed volcanic activity.en
dc.language.isoEnglishen
dc.relation.ispartofJ. Petrol.en
dc.relation.ispartofseries4 / 48 (2007)en
dc.subjectSomma^Vesuviusen
dc.subjectcrustal contaminationen
dc.subjectsource heterogeneityen
dc.subjectradiogenic and stable isotopesen
dc.titleMagmatic History of Somma^Vesuvius on the Basis of New Geochemical and Isotopic Data from a Deep Borehole (Camaldoli dellaTorre)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber753-784en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.05. Mineralogy and petrologyen
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.10. Stratigraphyen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.05. Volcanic rocksen
dc.identifier.doi10.1093/petrology/egl081en
dc.relation.referenceswith 87Sr/86Sr (Fig. 12b), action of the mantle source ized by relatively high ted sediments, progressively ctions proceed, meet these d1 B plot corroborates the urce contamination from Vesuvius and Campi ’Antonio et al., 2007). opic studies of the Plinian, Somma^Vesuvius eruptions a mixing processes before processes are well documen-ariations in the magmas he eruptions and by isotopic et al., 1991a; Civetta & al., 1993; Cioni et al., 1995). mixing processes was not efore we have not collected . The occurrence of such T rocks, is probably shown ria between clinopyroxene one shoshonitic and one ble 2). ontamination and source e main factors required to with distinct isotopic t towards the surface, mix graphic reconstruction of a maldoli della Torre, and of isotopic investigations on d us to shed light on the of its magmatic system. formation of the Somma^ lacement of trachytic pyro-egraean and local origin, he catastrophic Campanian 9 ka, the earliest Somma^ s characterized by a few ch formed a now unexposed la Torre area, followed by ted by the development of ly, volcanism resulted in a in composition through time ite, shoshonite again and led to the formation of the most of the more recent of phonotephritic lavas, ka, changes the current view that strongly undersaturated tephritic magmas were erupted only in the last 4 kyr of Somma^Vesuvius history. The isotopic variations result from both source heteroge-neity and crustal assimilation at mid-crustal depth. During ascent to the surface and stagnation at mid-crustal levels, the Vesuvian magmas interacted either with Hercynian continental crust or, possibly, with Mesozoic limestone. Contamination by Hercynian crust satisfactorily explains the isotopic variation over the transition shoshonite^latite, with 2% assimilation and 18% crystallization, according to EC-AFC calculations. The transition shoshonite^phonotephrite could possibly be the result of contamination by Mesozoic limestone. This process is not yet well constrained and more experimental data are necessary to assess the role of limestone contami-nation in the genesis of strongly undersaturated magmas at Vesuvius. At shallower depths isotopically distinct magmas, mostly resulting from contamination, differentiate and mix, lead-ing to the isotopic range of Vesuvian products. ACKNOWLEDGEMENTS The authors wish to thank F. Spera and R. Moretti for their kind help in EC-AFC and MELTS modelling. P. 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dc.description.obiettivoSpecifico2.3. TTC - Laboratori di chimica e fisica delle rocceen
dc.description.obiettivoSpecifico3.5. Geologia e storia dei sistemi vulcanicien
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorDi Renzo, V.en
dc.contributor.authorDi Vito, M. A.en
dc.contributor.authorArienzo, I.en
dc.contributor.authorCarandente, A.en
dc.contributor.authorCivetta, L.en
dc.contributor.authorD'Antonio, M.en
dc.contributor.authorGiordano, F.en
dc.contributor.authorOrsi, G.en
dc.contributor.authorTonarini, S.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
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crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptUniversità di Napoli "Federico II"-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
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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-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
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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.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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