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      The effects of local variations in conditions on carbon storage and release in the continental mantle

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          ABSTRACT

          Recent advances indicate that the amount of carbon released by gradual degassing from the mantle needs to be revised upwards, whereas the carbon supplied by plumes may have been overestimated in the past. Variations in rock types and oxidation state may be very local and exert strong influences on carbon storage and release mechanisms. Deep subduction may be prevented by diapirism in thick sedimentary packages, whereas carbonates in thinner sequences may be subducted. Carbonates stored in the mantle transition zone will melt when they heat up, recognized by coupled stable isotope systems (e.g. Mg, Zn, Ca). There is no single ‘mantle oxygen fugacity’, particularly in the thermal boundary layer (TBL) and lowermost lithosphere, where very local mixtures of rock types coexist. Carbonate-rich melts from either subduction or melting of the uppermost asthenosphere trap carbon by redox freezing or as carbonate-rich dykes in this zone. Deeply derived, reduced melts may form further diamond reservoirs, recognized as polycrystalline diamonds associated with websteritic silicate minerals. Carbon is released by either edge-driven convection, which tears sections of the TBL and lower lithosphere down so that they melt by a mixture of heating and oxidation, or by lateral advection of solids beneath rifts. Both mechanisms operate at steps in lithosphere thickness and result in carbonate-rich melts, explaining the spatial association of craton edges and carbonate-rich magmatism. High-pressure experiments on individual rock types, and increasingly on reactions between rocks and melts, are fine-tuning our understanding of processes and turning up unexpected results that are not seen in studies of single rocks. Future research should concentrate on elucidating local variations and integrating these with the interpretation of geophysical signals. Global concepts such as average sediment compositions and a uniform mantle oxidation state are not appropriate for small-scale processes; an increased focus on local variations will help to refine carbon budget models.

          Abstract

          Carbon is moved around in the Earth’s mantle in melts and fluids. This review shows that accurate estimations of the amount of carbon moved must consider local variations in temperature, oxidation state, and rock types deep in the mantle.

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          Implications of mantle plume structure for the evolution of flood basalts

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            The global range of subduction zone thermal models

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                Author and article information

                Contributors
                Journal
                Natl Sci Rev
                Natl Sci Rev
                nsr
                National Science Review
                Oxford University Press
                2095-5138
                2053-714X
                June 2024
                18 March 2024
                18 March 2024
                : 11
                : 6
                : nwae098
                Affiliations
                School of Natural Sciences, Macquarie University , North Ryde 2109, New South Wales, Australia
                Research School of Earth Sciences, Australian National University , Canberra, AT 2601, Australia
                School of Natural Sciences, Macquarie University , North Ryde 2109, New South Wales, Australia
                State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences , Wuhan 430074, China
                Research School of Earth Sciences, Australian National University , Canberra, AT 2601, Australia
                Author notes
                Corresponding author. E-mail: stephen.foley@ 123456mq.edu.au
                Article
                nwae098
                10.1093/nsr/nwae098
                11203914
                38933600
                57b2cf1d-9392-4389-a2f5-cd0018001627
                © The Author(s) 2024. Published by Oxford University Press on behalf of China Science Publishing & Media Ltd.

                This is an Open Access article distributed under the terms of the Creative Commons Attribution License ( https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

                History
                : 09 December 2023
                : 11 March 2024
                : 12 March 2024
                : 26 June 2024
                Page count
                Pages: 15
                Funding
                Funded by: Australian Research Council, DOI 10.13039/501100000923;
                Award ID: FL180100134
                Award ID: DP210101268
                Categories
                REVIEW
                EARTH SCIENCES
                Special Topic: Origin and Cycling of Volatiles in Habitable Planets
                Nsr/9
                AcademicSubjects/MED00010
                AcademicSubjects/SCI00010

                lithospheric mantle,carbonate melts,deep carbon cycle,craton destruction,continental rifts

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