Uncovering and quantifying the subduction zone sulfur cycle from the slab perspective.
basic_science · Level V
Where this comes from
- Record sourced from PubMed, PMID 31980597.
- Also identified by DOI 10.1038/s41467-019-14110-4 and PMC identifier 6981181.
- Licence recorded as CC BY.
- The licence permits redistribution, so the abstract is shown in full and the full text is available from the publisher.
Abstract
Sulfur belongs among H<sub>2</sub>O, CO<sub>2</sub>, and Cl as one of the key volatiles in Earth's chemical cycles. High oxygen fugacity, sulfur concentration, and δ<sup>34</sup>S values in volcanic arc rocks have been attributed to significant sulfate addition by slab fluids. However, sulfur speciation, flux, and isotope composition in slab-dehydrated fluids remain unclear. Here, we use high-pressure rocks and enclosed veins to provide direct constraints on subduction zone sulfur recycling for a typical oceanic lithosphere. Textural and thermodynamic evidence indicates the predominance of reduced sulfur species in slab fluids; those derived from metasediments, altered oceanic crust, and serpentinite have δ<sup>34</sup>S values of approximately -8‰, -1‰, and +8‰, respectively. Mass-balance calculations demonstrate that 6.4% (up to 20% maximum) of total subducted sulfur is released between 30-230 km depth, and the predominant sulfur loss takes place at 70-100 km with a net δ<sup>34</sup>S composition of -2.5 ± 3‰. We conclude that modest slab-to-wedge sulfur transport occurs, but that slab-derived fluids provide negligible sulfate to oxidize the sub-arc mantle and cannot deliver <sup>34</sup>S-enriched sulfur to produce the positive δ<sup>34</sup>S signature in arc settings. Most sulfur has negative δ<sup>34</sup>S and is subducted into the deep mantle, which could cause a long-term increase in the δ<sup>34</sup>S of Earth surface reservoirs.