EGU24-9886, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-9886
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Sulfur disproportionation in sub-arc COHS slab fluids drives mantle wedge oxidation

Andrea Maffeis1, Maria Luce Frezzotti2, James Alexander Denis Connolly3, Daniele Castelli1, and Simona Ferrando1
Andrea Maffeis et al.
  • 1Università di Torino, Dipartimento di Scienze della Terra, Italy (andrea.maffeis@unito.it)
  • 2Università degli Studi di Milano-Bicocca, Dipartimento di Scienze dell’Ambiente e della Terra
  • 3ETH Zurich, Department of Earth Sciences, Institute for Geochemistry and Petrology

Sulfur degassed at volcanic arcs calls for dissolved S6+ released by subduction-zone fluids, oxidising (in association with C) the sub-arc mantle, but sulfur speciation in subduction fluids at subarc depths remains unclear. We apply electrolytic fluid thermodynamics to model the dissolution behaviour of pyrite in meta-carbonate sediments as a function of P, T and rock redox state up to 4.3 GPa and 730°C. At subarc depth and at the redox conditions of the fayalite-magnetite-quartz oxygen buffer, pyrite dissolution releases oxidised S in fluids by disproportionation into sulfate, bisulfite, and sulfide species. These findings indicate that oxidised, sulfur-rich COHS fluids form within subducting slabs at depths greater than 100 km independent from slab redox state and that sulfur can be more effective than the concomitantly dissolved carbon at oxidising the mantle wedge, especially when carbonates are stable in the mantle. Further open system modelling shows that such fluids are capable of oxidising the sub-arc mantle within a few million years.

How to cite: Maffeis, A., Frezzotti, M. L., Connolly, J. A. D., Castelli, D., and Ferrando, S.: Sulfur disproportionation in sub-arc COHS slab fluids drives mantle wedge oxidation, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-9886, https://doi.org/10.5194/egusphere-egu24-9886, 2024.