Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6653
AuthorsPappalardo, L.* 
Mastrolorenzo, G.* 
TitleShort residence times for alkaline Vesuvius magmas in a multi-depth supply system: Evidence from geochemical and textural studies
Issue Date2010
Series/Report no./296 (2010)
DOI10.1016/j.epsl.2010.05.010
URIhttp://hdl.handle.net/2122/6653
Keywordsresidence time
phonolite
Vesuvius
Subject Classification04. Solid Earth::04.01. Earth Interior::04.01.04. Mineral physics and properties of rocks 
04. Solid Earth::04.04. Geology::04.04.05. Mineralogy and petrology 
04. Solid Earth::04.04. Geology::04.04.07. Rock geochemistry 
04. Solid Earth::04.04. Geology::04.04.10. Stratigraphy 
AbstractIt is crucial to understand magma chamber chemico-physical conditions and residence times for high-risk volcanoes because these factors control the occurrence and size of future eruptions. In order to define magmatic pressure–temperature conditions and residence times at the Somma–Vesuvius volcano, we studied the geochemistry and texture of selected past eruptions that are representative of the entire volcanic history. Our petrological model indicates a multi-depth magma chamber composed of a deeper tephritic (350– 400 Mpa) magma layer, which fed Strombolian and effusive eruptions during open-conduit activity, and an upper (200–250 Mpa) phonolitic level, which supplied the high explosive events that followed closedconduit repose time. This upper reservoir matches the inferred transition between sedimentary sequences and metamorphic basement. At this level, the presence of a structural and lithological discontinuity favors magma storage during closed-conduit periods. The prevalent differentiation process was fractional crystallization during the magma cooling associated with upward migration of less dense, evolved liquids. Our results indicate that major steam exolution occurred during the late crystallization stage of phonolites, which accounts for the high Volcanic Explosivity Index (VEI) of eruptions supplied by these melts. Moreover, our phenocryst CSD data reveal the rapid crystallization and differentiation (decades to centuries) of alkaline Somma–Vesuvius magmas. This implies that the 400 km2 partial melting zone detected by tomography studies at 8–10 km depth beneath Vesuvius should consist of differentiated magma that is already capable of generating a large-scale (plinian) explosive event if renewed activity develops out of the present closed-conduit state. Additionally, because our microlite CSD data indicate rapid magma migration from the chamber toward the surface, precursory activity could appear only short time before a major eruption.
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