Abstract

We present an empirical model of sulphur solubility that allows us to calculate f S2 if P, T, fO2 and the melt composition, including H2O and S, are known. The model is calibrated against three main experimental data bases consisting in both dry and hydrous silicate melts. Its prime goal is to calculate the f S2 of hydrous basalts that currently lack experimental constraints of their sulphur solubility behaviour. Application of the model to Stromboli, Vesuvius, Vulcano and Etna eruptive products shows that the primitive magmas found at these volcanoes record f S2 in the range 0.1-1 bar. In contrast, at all volcanoes the magmatic evolution is marked by dramatic variations in f S2 that spreads over up to 9 orders of magnitude. The f S2 can either increase during differentiation or decrease during decompression to shallow reservoirs, and seems to be related to closed versus open conduit conditions, respectively. The calculated f S2 shows that the Italian magmas are undersaturated in a FeS melt, except during closed conduit conditions, in which case differentiation may eventually reach conditions of sulphide melt saturation. The knowledge of f S2, fO2 and fH2O allows us to calculate the fluid phase composition coexisting with magmas at depth in the C-O-H-S system. Calculated fluids show a wide range in composition, with CO2 mole fractions of up to 0.97. Except at shallow levels, the fluid phase is generally dominated by CO2 and H2O species, the mole fractions of SO2 and H2S rarely exceeding 0.05 each. The comparison between calculated fluid compositions and volcanic gases shows that such an approach should provide constraints on both the depth and mode of degassing, as well as on the amount of free fluid in magma reservoirs. Under the assumption of a single step separation of the gas phase in a closed-system condition, the application to Stromboli and Etna suggests that the main reservoirs feeding the eruptions and persistent volcanic plumes at these volcanoes might contain as much as 5 wt% of a free fluid phase. Consideration of the magma budget needed to balance the amounts of volatiles emitted in the light of these results shows that the amount of nonerupted magma could be overestimated by as much as one order of magnitude.

Highlights

  • The determination of the composition of the fluids that coexist with magmas at depth requires1) a good definition of the magma pre-eruptive conditions (P, T, f O2, f S2, f H2O) and 2) solubility models for the main volatile species

  • For any volatile species dissolved in a silicate melt that is saturated in a fluid, equilibrium conditions demand that the fugacity fi of species i in the melt equals its fugacity in the fluid

  • Of the work done at high pressure, only that of Luhr (1990) provides sulphur solubility data obtained under known f S2 estimated from either Fe-FeS equilibria or equilibrium assemblages involving anhydrite

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Summary

Introduction

The determination of the composition of the fluids that coexist with magmas at depth requires. 1) a good definition of the magma pre-eruptive conditions (P, T, f O2, f S2, f H2O) and 2) solubility models for the main volatile species The combination of these two sets of information allows us to calculate the fluid composition through the consideration of fluid-melt equilibria (e.g., Scaillet and Evans, 1999). Of the work done at high pressure, only that of Luhr (1990) provides sulphur solubility data obtained under known f S2 estimated from either Fe-FeS equilibria or equilibrium assemblages involving anhydrite It is this mid-compositional range of hydrous mafic to intermediate magmas that still lacks experimental coverage, and this is unfortunate because most of arc magmas belong to this category. The combination of the two sets of data (calculation and observation) should allow a better use of volcanic gases as monitoring tools during on-going volcanic crisis

An empirical model for hydrous basaltic melts
Calculation of fluid phase composition
Source of data
Stromboli
Vesuvius
Vulcano
Trends in f S2 and sulphide saturation
Composition of fluids
Findings
Discussion and conclusions
Full Text
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