24
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: found
      • Article: found
      Is Open Access

      Subducting serpentinites release reduced, not oxidized, aqueous fluids

      research-article

      Read this article at

      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Abstract

          The observation that primitive arc magmas are more oxidized than mid-ocean-ridge basalts has led to the paradigm that slab-derived fluids carry SO 2 and CO 2 that metasomatize and oxidize the sub-arc mantle wedge. We combine petrography and thermodynamic modelling to quantify the oxygen fugacity ( fO 2) and speciation of the fluids generated by serpentinite dehydration during subduction. Silicate-magnetite assemblages maintain fO 2 conditions similar to the quartz-fayalite-magnetite (QFM) buffer at fore-arc conditions. Sulphides are stable under such conditions and aqueous fluids contain minor S. At sub-arc depth, dehydration occurs under more reducing conditions producing aqueous fluids carrying H 2S. This finding brings into question current models in which serpentinite-derived fluids are the cause of oxidized arc magmatism and has major implications for the global volatile cycle, as well as for redox processes controlling subduction zone geodynamics.

          Related collections

          Most cited references57

          • Record: found
          • Abstract: not found
          • Article: not found

          The global range of subduction zone thermal models

            Bookmark
            • Record: found
            • Abstract: found
            • Article: not found

            Serpentine stability to mantle depths and subduction-related magmatism.

            Results of high-pressure experiments on samples of hydrated mantle rocks show that the serpentine mineral antigorite is stable to approximately 720 degrees C at 2 gigapascals, to approximately 690 degrees C at 3 gigapascals, and to approximately 620 degrees C at 5 gigapascals. The breakdown of antigorite to forsterite plus enstatite under these conditions produces 13 percent H(2)O by weight to depths of 150 to 200 kilometers in subduction zones. This H(2)O is in an ideal position for ascent into the hotter, overlying mantle where it can cause partial melting in the source region for calc-alkaline magmas at a depth of 100 to 130 kilometers and a temperature of approximately 1300 degrees C. The breakdown of antigorite in hydrated mantle produces an order of magnitude more H(2)O than does the dehydration of altered oceanic crust.
              Bookmark
              • Record: found
              • Abstract: not found
              • Article: not found

              The redox states of basic and silicic magmas: a reflection of their source regions?

                Bookmark

                Author and article information

                Contributors
                francesca.piccoli@geo.unibe.ch
                Journal
                Sci Rep
                Sci Rep
                Scientific Reports
                Nature Publishing Group UK (London )
                2045-2322
                20 December 2019
                20 December 2019
                2019
                : 9
                : 19573
                Affiliations
                [1 ]ISNI 0000 0001 0726 5157, GRID grid.5734.5, University of Bern, Institute of Geological Sciences, ; Balzerstrasse 1+3, 3012 Bern, Switzerland
                [2 ]ISNI 0000 0001 2156 2780, GRID grid.5801.c, Department of Earth Science, , Swiss Federal Institute of Technology, ; Zurich, Switzerland
                Author information
                http://orcid.org/0000-0001-9941-0103
                http://orcid.org/0000-0001-5060-4281
                http://orcid.org/0000-0003-3296-3541
                Article
                55944
                10.1038/s41598-019-55944-8
                6925189
                31862932
                1b954243-bae7-4643-a839-db005801d8a7
                © The Author(s) 2019

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 1 August 2019
                : 5 December 2019
                Categories
                Article
                Custom metadata
                © The Author(s) 2019

                Uncategorized
                mineralogy,petrology
                Uncategorized
                mineralogy, petrology

                Comments

                Comment on this article