The geochemical evolution of the Mt. Somma-Vesuvius volcano

This work integrates new geochemical data with the numerous published analyses on rocks from the Mt. Somma-Vesuvius volcano. New quantitative models for the evolution of magma source regions and magma at different depths are proposed. The origin of the Somma-Vesuvius parental magma is modeled as 0.05–0.1 melt fractions of a MORB-type source composed of 54% olivine, 30% orthopyroxene, 10% clinopyroxene, 1% garnet, and 4% amphibole, and 1–5% sediment introduced through the adjacent arc system. The excess concentrations of Rb, Ba, K, and Sr are attributed to a subduction-related fluid phase. Major and trace element concentrations, coupled with Sr–Nd–Pb isotope signatures suggest that the bulk composition of sediments being subducted below southern Italy is similar to that of the carbonate rich sediment columns described by Plank and Langmuir (1998) and Vroon et al. (1995). Furthermore, it appears that the sediment contribution was introduced as a partial melt, which would account for some geochemical patterns, such as 143Nd/144Nd versus Th/Ce. The EC–AFC model (Spera and Bohrson, 2001) is then used to track the evolution of Somma-Vesuvius magmas. The results are consistent with the melting of crustal Hercynian basement at depths of 12 and >20 km (De Natale et al., 2001). Such a model is also consistent with the thermal model of Annen and Sparks (2002) for the evolution of magmatic provinces. Here, magmas from the upper mantle form a melt intrusion and storage zone at 12 to >20 km allowing for crustal melting to take place. At Vesuvius, Plinian eruptions involve the first magma withdrawn from a deep magma reservoir. Interplinian eruptions involve reduced volumes of magma stored over a larger depth range until the volcanic activity stops. This suggests that little magma is left in the melt intrusion and storage zone. A new cycle is started by a Plinian event when new magma rises from the upper mantle and is emplaced in the lower crust.