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      Large gem diamonds from metallic liquid in Earth's deep mantle.

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          Abstract

          The redox state of Earth's convecting mantle, masked by the lithospheric plates and basaltic magmatism of plate tectonics, is a key unknown in the evolutionary history of our planet. Here we report that large, exceptional gem diamonds like the Cullinan, Constellation, and Koh-i-Noor carry direct evidence of crystallization from a redox-sensitive metallic liquid phase in the deep mantle. These sublithospheric diamonds contain inclusions of solidified iron-nickel-carbon-sulfur melt, accompanied by a thin fluid layer of methane ± hydrogen, and sometimes majoritic garnet or former calcium silicate perovskite. The metal-dominated mineral assemblages and reduced volatiles in large gem diamonds indicate formation under metal-saturated conditions. We verify previous predictions that Earth has highly reducing deep mantle regions capable of precipitating a metallic iron phase that contains dissolved carbon and hydrogen.

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          Most cited references35

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          The deep carbon cycle and melting in Earth's interior

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            The Redox State of Earth's Mantle

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              Experimental evidence for the existence of iron-rich metal in the Earth's lower mantle.

              The oxidation state recorded by rocks from the Earth's upper mantle can be calculated from measurements of the distribution of Fe3+ and Fe2+ between the constituent minerals. The capacity for minerals to incorporate Fe3+ may also be a significant factor controlling the oxidation state of the mantle, and high-pressure experimental measurements of this property might provide important insights into the redox state of the more inaccessible deeper mantle. Here we show experimentally that the Fe3+ content of aluminous silicate perovskite, the dominant lower-mantle mineral, is independent of oxygen fugacity. High levels of Fe3+ are present in perovskite even when it is in chemical equilibrium with metallic iron. Silicate perovskite in the lower mantle will, therefore, have an Fe3+/total Fe ratio of at least 0.6, resulting in a whole-rock ratio of over ten times that of the upper mantle. Consequently, the lower mantle must either be enriched in Fe3+ or Fe3+ must form by the disproportionation of Fe2+ to produce Fe3+ plus iron metal. We argue that the lower mantle contains approximately 1 wt% of a metallic iron-rich alloy. The mantle's oxidation state and siderophile element budget have probably been influenced by the presence of this alloy.
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                Author and article information

                Journal
                Science
                Science (New York, N.Y.)
                American Association for the Advancement of Science (AAAS)
                1095-9203
                0036-8075
                Dec 16 2016
                : 354
                : 6318
                Affiliations
                [1 ] Gemological Institute of America, New York, NY 10036, USA. evan.smith@gia.edu.
                [2 ] Department of Terrestrial Magnetism, Carnegie Institution for Science, Washington, DC 20015, USA.
                [3 ] Department of Geosciences, University of Padova, Padova 35131, Italy.
                [4 ] Geophysical Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.
                [5 ] Department of Geological Sciences, University of Cape Town, Rondebosch 7701, South Africa.
                [6 ] Gemological Institute of America, New York, NY 10036, USA.
                Article
                354/6318/1403
                10.1126/science.aal1303
                27980206
                fa673c43-f0ee-4ad8-80ad-97f6d2267561
                History

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