Petrology,geochemistry and Sr-isotope characteristics of lavas from the area of Commenda (Mts. Vulsini,Italy) |
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Authors: | L. Civetta P. Del Carmine P. Manetti A. Peccerillo G. Poli |
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Affiliation: | (1) Dipartimento di Geofisica e Vulcanologia, Università di Napoli, Italy;(2) I.N.F.N., Sezione di Firenze, Firenze, Italy;(3) Dipartimento di Scienze della Terra, Università di Firenze, Italy |
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Abstract: | Major, trace element and Sr-isotope compositions are reported for a suite of lavas coming from the area of Commenda in the SE Vulsinian district. The analyzed samples have all low silica contents and variable but generally high CaO, MgO and FeOt. Based on K2O% and K2O/Na2O ratio, the rocks from Commenda can be classified as belonging to the Potassic Series (KS) and the High-potassium Series (HKS). The HKS rocks appear to have derived by cristal/liquid fractionation from the most mafic types with separation of olivine and clinopyroxene and then of clinopyroxene + leucite. The most primitive HKS rocks have aphyric texture and high Mg-values, Cr and Ni contents which are close or within the range of values of magmas formed by partial melting of periodititic mantle sources. The KS rocks have lower incompatible element contents as the HKS rocks with similar degree of evolution.The variations of Sr-isotopic ratios of the analyzed rocks and of other Vulsinian lavas, indicate that the basic HKS Vulsinian rocks did not interact significantly with the continental crust. Instead, the KS appears to have evolved by combined crystal fractionation and assimilation processes, starting from parental magmas which had87Sr/86Sr ratio not significantly lower than that found in the less evolved rocks of the suite.The most primitive HKS rocks from Commenda have hygromagmatophile element distribution pattern characterized by high ratio of LILE/HFSE with negative anomalies of Ta and Ti, resembling closely those of other Roman mafic volcanics. The primitive geochemical characteristics of the Commenda rocks exclude that these features are the products of interaction with the crust and provide a further support to the hypothesis of a genesis within a subduction-modified mantle source. |
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