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Sulfur-enriched sub-arc fluids drive deep sulfur cycling in subduction zones
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  • Published: 07 April 2026

Sulfur-enriched sub-arc fluids drive deep sulfur cycling in subduction zones

  • Dong-Bo Tan1,
  • Yilin Xiao  ORCID: orcid.org/0000-0002-5309-07111,2,
  • Yibing Li  ORCID: orcid.org/0000-0003-0111-47233,
  • Haiyang Liu  ORCID: orcid.org/0000-0002-7055-34824,
  • Deshi Jin1,
  • Yang-Yang Wang1,
  • Xiaoguang Li  ORCID: orcid.org/0000-0001-6853-24585,
  • Haihao Guo6,
  • Zeng-Li Guo7,
  • Carlos J. Garrido  ORCID: orcid.org/0000-0003-4357-36378 &
  • …
  • Timothy Kusky  ORCID: orcid.org/0000-0002-4553-620X6 

Nature Communications , Article number:  (2026) Cite this article

We are providing an unedited version of this manuscript to give early access to its findings. Before final publication, the manuscript will undergo further editing. Please note there may be errors present which affect the content, and all legal disclaimers apply.

Subjects

  • Geochemistry
  • Geodynamics
  • Volcanology

Abstract

Arc magmas are enriched in sulfur relative to mid-ocean ridge basalts, commonly attributed to slab-derived sulfur inputs during subduction. However, the contribution of slab fluids remains debated because sulfur concentrations in sub-arc fluids have not been directly measured. Here we quantify sulfur in slab-derived fluids preserved as multiphase fluid inclusions composed of H2O, calcite, and chalcopyrite in omphacite from ultrahigh-pressure eclogites in the Sumdo orogenic belt. Three-dimensional Raman spectroscopy reveals high sulfur concentrations averaging ~6 wt.%. Mass-balance calculations indicate that such fluids can efficiently enrich the mantle wedge and supply up to ~70% of the sulfur emitted by arc volcanism. We further suggest that chalcopyrite formed through post-entrapment reduction of oxidized sulfur species by host omphacite, followed by precipitation with co-entrapped copper and iron. Our findings identify sub-arc depths as a critical window for slab sulfur release and provide key constraints on deep sulfur cycling and copper mobilization in arc systems.

Data availability

All data supporting the findings of this study are available in the Supplementary materials and in a public repository (Figshare) at https://figshare.com/s/56febb3cbcea3e8f0e45.

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Acknowledgements

This work was supported by the National Natural Science Foundation of China (grant 42230304 to Y.X., grant 42302050 to D.-B.T. and grant 42302053 to Y.-B.L.), the National Key Research and Development Program of China (2023YFF0807103 to H.-Y.L.), and the Taishan Scholar Program of Shandong (tsqn202507278 to H.-Y.L.). We thank Dr. Wancai Li, Tingting Xiao, and Rui Shi for assistance with the EPMA analyses.

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Authors and Affiliations

  1. State Key Laboratory of Lithospheric and Environmental Coevolution, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China

    Dong-Bo Tan, Yilin Xiao, Deshi Jin & Yang-Yang Wang

  2. Chinese Academy of Sciences Center of Excellence in Comparative Planetology, Hefei, China

    Yilin Xiao

  3. Marine Science and Technology College, Zhejiang Ocean University, Zhoushan, China

    Yibing Li

  4. Key Laboratory of Ocean Observation and Forecasting, Center of Deep Sea Research, Chinese Academy of Sciences, Qingdao, China

    Haiyang Liu

  5. State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China

    Xiaoguang Li

  6. State Key Laboratory of Geological Processes and Mineral Resources, School of Earth and Planetary Sciences, China University of Geosciences, Wuhan, China

    Haihao Guo & Timothy Kusky

  7. SK Lab-DeepMinE, MOE KLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China

    Zeng-Li Guo

  8. Instituto Andaluz de Ciencias de la Tierra (IACT–CSIC), CSIC, Granada, Spain

    Carlos J. Garrido

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Contributions

Y.X., D.-B.T. conceived and designed the study. Y.-Y.W., H.-H.G. collected the samples. D.-B.T., H.-Y.L., D.-S.J., and X.-G.L. performed the geochemical analyses. Z.-L.G. conducted the thermodynamic modeling. D.-B.T. wrote the initial draft of the manuscript. Y.X., Y.-B.L., Carlos J. Garrido, and Timothy Kusky contributed to manuscript revision. Funding was acquired by Y.X., D.-B.T., Y.-B. L., and H.-Y. L. All authors discussed the results and contributed to the final manuscript.

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Correspondence to Yilin Xiao.

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Tan, DB., Xiao, Y., Li, Y. et al. Sulfur-enriched sub-arc fluids drive deep sulfur cycling in subduction zones. Nat Commun (2026). https://doi.org/10.1038/s41467-026-71439-3

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  • Received: 17 September 2025

  • Accepted: 23 March 2026

  • Published: 07 April 2026

  • DOI: https://doi.org/10.1038/s41467-026-71439-3

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