Solubility and speciation of sulfur in silicate melts under crustal conditions

• Sulfide and sulfate capacities experimentally constrained in silicate melts at 1050 to 1250 °C. • The change in S 6+ /S 2− of a silicate melt with log f O 2 is strongly temperature dependent < 1200 °C. • Fe-S redox exchange may oxidise arc magmas by several log units in f O 2 as they crystallise. • Sulfide saturation is widespread in oxidised (> ΔFMQ +2) calc-alkaline magmas. • Cu-rich fluids should form by remobilising cumulate sulfides not sulfide-undersaturated melts. We have determined the solubility of sulfur as either sulfide (S 2− ) or sulfate (S 6+ ) in a wide range of silicate melts at 1 atm pressure and temperatures of 1050 to 1250 °C. The method involved suspension of the melt in either a mixture of CO 2 -CO-SO 2 (sulfide solubility) or SO 2 and air (sulfate solubility) for periods of up to 120 hours. Sulfur concentrations, measured by electron microprobe were converted into sulfide capacity C S 2 − and sulfate capacity C S 6 + using (Fincham and Richardson; 1954): log C S 2 − = log [ S 2 − ] + 1 2 log ( f S 2 f O 2 ) log C S 6 + = log [ SO 4 2 − ] − 1 2 log f S 2 − 3 2 log f O 2 [ S 2 − ] and [ SO 4 2 − ] refer to weight % sulfur dissolved in the melt as sulfate and sulfide respectively. Our new results demonstrate that extrapolation of earlier data to temperatures below 1200 °C yields good agreement for sulfide capacity but overestimates sulfate capacity. This means that sulfide is appreciably more stable relative to sulfate in crustal magmas (temperatures <1200 °C) than previously calculated. A major consequence is that the crossover from S 2− at low f O 2 to S 6+ at high f O 2 shifts upwards by ∼0.6 log f O 2 units relative to the FMQ buffer as temperature declines from 1200 °C to 1050 °C. The large temperature effect on sulfur speciation also means that there is electron exchange between Fe 2+ and S 6+ during magma cooling and ascent leading to high measured Fe 3+ /Fe 2+ in quenched melts, high calculated f O 2 and relatively reduced sulfur with high S 2− /S 6+ even at +2-3 log f O 2 units above the FMQ buffer. This self-oxidation mechanism at low temperatures is a major contribution to the observation that hydrous S-bearing arc magmas are more oxidised than MORB, which are generated at low f O 2 and which erupt at higher temperatures. Furthermore, these oxidised hydrous melts are sulfide saturated and should precipitate an Fe-rich sulfide throughout their path of ascent and differentiation in lower, mid and upper -crustal levels. Given that such sulfides would scavenge Cu and other chalcophile metals we suggest that the occurrence of Cu-(±Au) porphyry deposits is governed less by the capacity of magmas to remain Cu-rich, and more by the architecture and evolution of the cumulate pile, the timing and depth of volatile saturation, and the efficiency of Cl-rich fluids in later mobilisation of metals.

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Journal
Earth and Planetary Science Letters
Published
2026-05-09
DOI
https://doi.org/10.1016/j.epsl.2026.120088
Primary Topic
CO2 Sequestration and Geologic Interactions
Type
article
Field-Weighted Citation Impact
0.00

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article

Solubility and speciation of sulfur in silicate melts under crustal conditions

Lauren Gorojovsky, Bernard J. Wood
Earth and Planetary Science Letters
CO2 Sequestration and Geologic Interactions
article

Solubility and speciation of sulfur in silicate melts under crustal conditions

Lauren Gorojovsky, Bernard J. Wood
article en

Abstract

• Sulfide and sulfate capacities experimentally constrained in silicate melts at 1050 to 1250 °C. • The change in S 6+ /S 2− of a silicate melt with log f O 2 is strongly temperature dependent < 1200 °C. • Fe-S redox exchange may oxidise arc magmas by several log units in f O 2 as they crystallise. • Sulfide saturation is widespread in oxidised (> ΔFMQ +2) calc-alkaline magmas. • Cu-rich fluids should form by remobilising cumulate sulfides not sulfide-undersaturated melts. We have determined the solubility of sulfur as either sulfide (S 2− ) or sulfate (S 6+ ) in a wide range of silicate melts at 1 atm pressure and temperatures of 1050 to 1250 °C. The method involved suspension of the melt in either a mixture of CO 2 -CO-SO 2 (sulfide solubility) or SO 2 and air (sulfate solubility) for periods of up to 120 hours. Sulfur concentrations, measured by electron microprobe were converted into sulfide capacity C S 2 − and sulfate capacity C S 6 + using (Fincham and Richardson; 1954): log C S 2 − = log [ S 2 − ] + 1 2 log ( f S 2 f O 2 ) log C S 6 + = log [ SO 4 2 − ] − 1 2 log f S 2 − 3 2 log f O 2 [ S 2 − ] and [ SO 4 2 − ] refer to weight % sulfur dissolved in the melt as sulfate and sulfide respectively. Our new results demonstrate that extrapolation of earlier data to temperatures below 1200 °C yields good agreement for sulfide capacity but overestimates sulfate capacity. This means that sulfide is appreciably more stable relative to sulfate in crustal magmas (temperatures <1200 °C) than previously calculated. A major consequence is that the crossover from S 2− at low f O 2 to S 6+ at high f O 2 shifts upwards by ∼0.6 log f O 2 units relative to the FMQ buffer as temperature declines from 1200 °C to 1050 °C. The large temperature effect on sulfur speciation also means that there is electron exchange between Fe 2+ and S 6+ during magma cooling and ascent leading to high measured Fe 3+ /Fe 2+ in quenched melts, high calculated f O 2 and relatively reduced sulfur with high S 2− /S 6+ even at +2-3 log f O 2 units above the FMQ buffer. This self-oxidation mechanism at low temperatures is a major contribution to the observation that hydrous S-bearing arc magmas are more oxidised than MORB, which are generated at low f O 2 and which erupt at higher temperatures. Furthermore, these oxidised hydrous melts are sulfide saturated and should precipitate an Fe-rich sulfide throughout their path of ascent and differentiation in lower, mid and upper -crustal levels. Given that such sulfides would scavenge Cu and other chalcophile metals we suggest that the occurrence of Cu-(±Au) porphyry deposits is governed less by the capacity of magmas to remain Cu-rich, and more by the architecture and evolution of the cumulate pile, the timing and depth of volatile saturation, and the efficiency of Cl-rich fluids in later mobilisation of metals.

Earth and Planetary Science LettersVol. 687
University of Oxford (GB)
UK Research and Innovation
Openalex Percentile: Top 8%
CO2 Sequestration and Geologic Interactions
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