Phase Equilibria Constraints on the Chemical and Physical Evolution of the Campanian Ignimbrite

نویسندگان

  • SARAH J. FOWLER
  • HARVEY E. BELKIN
  • BENEDETTO DE VIVO
چکیده

The Campanian Ignimbrite is a 4200 km trachyte^phonolite pyroclastic deposit that erupted at 39 3 0 1ka within the Campi Flegrei west of Naples, Italy. Here we test the hypothesis that Campanian Ignimbrite magma was derived by isobaric crystal fractionation of a parental basaltic trachyandesitic melt that reacted and came into local equilibrium with small amounts (5^10 wt%) of crustal rock (skarns and foid-syenites) during crystallization. Comparison of observed crystal and magma compositions with results of phase equilibria assimilation^fractionation simulations (MELTS) is generally very good. Oxygen fugacity was approximately buffered along QFMþ1 (where QFM is the quartz^ fayalite^magnetite buffer) during isobaric fractionation at 0 15 GPa ( 6 km depth).The parental melt, reconstructed from melt inclusion and host clinopyroxene compositions, is found to be basaltic trachyandesite liquid (51 1 wt% SiO2, 9 3 wt% MgO, 3 wt% H2O). A significant feature of phase equilibria simulations is the existence of a pseudo-invariant temperature, 883 8C, at which the fraction of melt remaining in the system decreases abruptly from 0 5 to50 1. Crystallization at the pseudo-invariant point leads to abrupt changes in the composition, properties (density, dissolved water content), and physical state (viscosity, volume fraction fluid) of melt and magma. A dramatic decrease in melt viscosity (from 1700 Pa s to 200 Pa s), coupled with a change in the volume fraction of water in magma (from 0 1 to 0 8) and a dramatic decrease in melt and magma density acted as a destabilizing eruption trigger. Thermal models suggest a timescale of 200 kyr from the beginning of fractionation until eruption, leading to an apparent rate of evolved magma generation of about 10 3 km/year. In situ crystallization and crystal settling in density-stratified regions, as well as in convectively mixed, less evolved subjacent magma, operate rapidly enough to match this apparent volumetric rate of evolved magma production.

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تاریخ انتشار 2006