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      Pressure stabilizes ferrous iron in bridgmanite under hydrous deep lower mantle conditions

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          Abstract

          Earth’s lower mantle is a potential water reservoir. The physical and chemical properties of the region are in part controlled by the Fe 3+/ΣFe ratio and total iron content in bridgmanite. However, the water effect on the chemistry of bridgmanite remains unclear. We carry out laser-heated diamond anvil cell experiments under hydrous conditions and observe dominant Fe 2+ in bridgmanite (Mg, Fe)SiO 3 above 105 GPa under the normal geotherm conditions corresponding to depth > 2300 km, whereas Fe 3+-rich bridgmanite is obtained at lower pressures. We further observe FeO in coexistence with hydrous NiAs-type SiO 2 under similar conditions, indicating that the stability of ferrous iron is a combined result of H 2O effect and high pressure. The stability of ferrous iron in bridgmanite under hydrous conditions would provide an explanation for the nature of the low-shear-velocity anomalies in the deep lower mantle. In addition, entrainment from a hydrous dense layer may influence mantle plume dynamics and contribute to variations in the redox conditions of the mantle.

          Abstract

          The large low-shear-velocity anomalies in the deep lower mantle below 2300 km depth may relate to H 2O-induced ferrous iron stability in bridgmanite, according to laser-heated diamond anvil cell experiments.

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          Most cited references61

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          Degree 12 model of shear velocity heterogeneity in the mantle

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            Rheology of synthetic olivine aggregates: Influence of grain size and water

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              Broad plumes rooted at the base of the Earth's mantle beneath major hotspots

              Plumes of hot upwelling rock rooted in the deep mantle have been proposed as a possible origin of hotspot volcanoes, but this idea is the subject of vigorous debate. On the basis of geodynamic computations, plumes of purely thermal origin should comprise thin tails, only several hundred kilometres wide, and be difficult to detect using standard seismic tomography techniques. Here we describe the use of a whole-mantle seismic imaging technique--combining accurate wavefield computations with information contained in whole seismic waveforms--that reveals the presence of broad (not thin), quasi-vertical conduits beneath many prominent hotspots. These conduits extend from the core-mantle boundary to about 1,000 kilometres below Earth's surface, where some are deflected horizontally, as though entrained into more vigorous upper-mantle circulation. At the base of the mantle, these conduits are rooted in patches of greatly reduced shear velocity that, in the case of Hawaii, Iceland and Samoa, correspond to the locations of known large ultralow-velocity zones. This correspondence clearly establishes a continuous connection between such zones and mantle plumes. We also show that the imaged conduits are robustly broader than classical thermal plume tails, suggesting that they are long-lived, and may have a thermochemical origin. Their vertical orientation suggests very sluggish background circulation below depths of 1,000 kilometres. Our results should provide constraints on studies of viscosity layering of Earth's mantle and guide further research into thermochemical convection.
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                Author and article information

                Contributors
                zhangli@hpstar.ac.cn
                Journal
                Nat Commun
                Nat Commun
                Nature Communications
                Nature Publishing Group UK (London )
                2041-1723
                21 May 2024
                21 May 2024
                2024
                : 15
                : 4333
                Affiliations
                [1 ]GRID grid.410733.2, Center for High Pressure Science and Technology Advanced Research, ; Shanghai, China
                [2 ]Shanghai Key Laboratory MFree, Institute for Shanghai Advanced Research in Physical Sciences, Shanghai, China
                Author information
                http://orcid.org/0000-0003-2684-6832
                http://orcid.org/0000-0003-3920-744X
                http://orcid.org/0000-0002-7114-0647
                http://orcid.org/0000-0002-6213-4472
                http://orcid.org/0000-0002-0481-5683
                Article
                48665
                10.1038/s41467-024-48665-8
                11109188
                38773099
                c377b86c-300c-4398-88b3-f58eb67c0fd8
                © The Author(s) 2024

                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 licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence 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 licence, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 19 June 2023
                : 9 May 2024
                Funding
                Funded by: FundRef https://doi.org/10.13039/501100001809, National Natural Science Foundation of China (National Science Foundation of China);
                Award ID: 42150103
                Award ID: U2230401
                Award Recipient :
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                © Springer Nature Limited 2024

                Uncategorized
                mineralogy,geochemistry,geodynamics
                Uncategorized
                mineralogy, geochemistry, geodynamics

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