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      Silicate dissolution boosts the CO 2 concentrations in subduction fluids

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          Abstract

          Estimates of dissolved CO 2 in subduction-zone fluids are based on thermodynamic models, relying on a very sparse experimental data base. Here, we present experimental data at 1–3 GPa, 800 °C, and ∆FMQ ≈ −0.5 for the volatiles and solute contents of graphite-saturated fluids in the systems COH, SiO 2–COH ( + quartz/coesite) and MgO–SiO 2–COH ( + forsterite and enstatite). The CO 2 content of fluids interacting with silicates exceeds the amounts measured in the pure COH system by up to 30 mol%, as a consequence of a decrease in water activity probably associated with the formation of organic complexes containing Si–O–C and Si–O–Mg bonds. The interaction of deep aqueous fluids with silicates is a novel mechanism for controlling the composition of subduction COH fluids, promoting the deep CO 2 transfer from the slab–mantle interface to the overlying mantle wedge, in particular where fluids are stable over melts.

          Abstract

          Current estimates of dissolved CO 2 in subduction-zone fluids based on thermodynamic models rely on a very sparse experimental data base. Here, the authors show that experimental graphite-saturated COH fluids interacting with silicates at 1–3 GPa and 800 °C display unpredictably high CO 2 contents.

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          Trace element signature of subduction-zone fluids, melts and supercritical liquids at 120-180 km depth.

          Fluids and melts liberated from subducting oceanic crust recycle lithophile elements back into the mantle wedge, facilitate melting and ultimately lead to prolific subduction-zone arc volcanism. The nature and composition of the mobile phases generated in the subducting slab at high pressures have, however, remained largely unknown. Here we report direct LA-ICPMS measurements of the composition of fluids and melts equilibrated with a basaltic eclogite at pressures equivalent to depths in the Earth of 120-180 km and temperatures of 700-1,200 degrees C. The resultant liquid/mineral partition coefficients constrain the recycling rates of key elements. The dichotomy of dehydration versus melting at 120 km depth is expressed through contrasting behaviour of many trace elements (U/Th, Sr, Ba, Be and the light rare-earth elements). At pressures equivalent to 180 km depth, however, a supercritical liquid with melt-like solubilities for the investigated trace elements is observed, even at low temperatures. This mobilizes most of the key trace elements (except the heavy rare-earth elements, Y and Sc) and thus limits fluid-phase transfer of geochemical signatures in subduction zones to pressures less than 6 GPa.
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            Reevaluating carbon fluxes in subduction zones, what goes down, mostly comes up.

            Carbon fluxes in subduction zones can be better constrained by including new estimates of carbon concentration in subducting mantle peridotites, consideration of carbonate solubility in aqueous fluid along subduction geotherms, and diapirism of carbon-bearing metasediments. Whereas previous studies concluded that about half the subducting carbon is returned to the convecting mantle, we find that relatively little carbon may be recycled. If so, input from subduction zones into the overlying plate is larger than output from arc volcanoes plus diffuse venting, and substantial quantities of carbon are stored in the mantle lithosphere and crust. Also, if the subduction zone carbon cycle is nearly closed on time scales of 5-10 Ma, then the carbon content of the mantle lithosphere + crust + ocean + atmosphere must be increasing. Such an increase is consistent with inferences from noble gas data. Carbon in diamonds, which may have been recycled into the convecting mantle, is a small fraction of the global carbon inventory.
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              Melting in the Earth's deep upper mantle caused by carbon dioxide.

              The onset of partial melting beneath mid-ocean ridges governs the cycling of highly incompatible elements from the mantle to the crust, the flux of key volatiles (such as CO2, He and Ar) and the rheological properties of the upper mantle. Geophysical observations indicate that melting beneath ridges begins at depths approaching 300 km, but the cause of this melting has remained unclear. Here we determine the solidus of carbonated peridotite from 3 to 10 GPa and demonstrate that melting beneath ridges may occur at depths up to 330 km, producing 0.03-0.3% carbonatite liquid. We argue that these melts promote recrystallization and realignment of the mineral matrix, which may explain the geophysical observations. Extraction of incipient carbonatite melts from deep within the oceanic mantle produces an abundant source of metasomatic fluids and a vast mantle residue depleted in highly incompatible elements and fractionated in key parent-daughter elements. We infer that carbon, helium, argon and highly incompatible heat-producing elements (such as uranium, thorium and potassium) are efficiently scavenged from depths of approximately 200-330 km in the upper mantle.
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                Author and article information

                Contributors
                simone.tumiati@unimi.it
                Journal
                Nat Commun
                Nat Commun
                Nature Communications
                Nature Publishing Group UK (London )
                2041-1723
                20 September 2017
                20 September 2017
                2017
                : 8
                : 616
                Affiliations
                [1 ]ISNI 0000 0004 1757 2822, GRID grid.4708.b, Dipartimento di Scienze della Terra, , Università degli Studi di Milano, ; via Mangiagalli 34, 20133 Milano, Italy
                [2 ]ISNI 0000 0001 2174 1754, GRID grid.7563.7, Dipartimento di Scienze dell’Ambiente e della Terra, , Università degli Studi di Milano Bicocca, ; Piazza della Scienza 4, 20126 Milano, Italy
                [3 ]ISNI 0000 0001 2171 9311, GRID grid.21107.35, Department of Earth & Planetary Sciences, , Johns Hopkins University, ; Baltimore, MD 21218 USA
                [4 ]ISNI 0000 0001 0726 5157, GRID grid.5734.5, Institute of Geological Sciences, , University of Bern, ; Baltzerstrasse 1+3, 3012 Bern, Switzerland
                [5 ]ISNI 0000000121724807, GRID grid.18147.3b, Dipartimento di Scienza e Alta Tecnologia, , Università degli Studi dell’Insubria, ; via Valleggio 11, 22100 Como, Italy
                [6 ]Institute of Geochemistry and Petrology, ETH Zürich, Clausiusstrasse 25 / NW E77, 8092 Zürich, Switzerland
                [7 ]ISNI 0000 0001 2308 1657, GRID grid.462844.8, Institut de Minéralogie, de Physique des Matériaux, et de Cosmochimie (IMPMC), , Sorbonne Universités – UPMC, ; UMR CNRS, 7590, Muséum National d’Histoire Naturelle, IRD UMR 206, 75005 Paris, France
                Author information
                http://orcid.org/0000-0003-0900-6145
                http://orcid.org/0000-0001-5313-1678
                Article
                562
                10.1038/s41467-017-00562-z
                5606994
                28931819
                d0d7414b-63ef-497e-b143-6d391d9c2669
                © The Author(s) 2017

                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
                : 11 November 2015
                : 5 July 2017
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