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      Core formation and the oxidation state of the Earth

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      Earth and Planetary Science Letters
      Elsevier BV

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          Rapid accretion and early core formation on asteroids and the terrestrial planets from Hf–W chronometry

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            The chemical composition of the Earth

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              Models of the Earth's Core.

              Combined inferences from seismology, high-pressure experiment and theory, geomagnetism, fluid dynamics, and current views of terrestrial planetary evolution lead to models of the earth's core with the following properties. Core formation was contemporaneous with earth accretion; the core is not in chemical equilibrium with the mantle; the outer core is a fluid iron alloy containing significant quantities of lighter elements and is probably almost adiabatic and compositionally uniform; the more iron-rich inner solid core is a consequence of partial freezing of the outer core, and the energy release from this process sustains the earth's magnetic field; and the thermodynamic properties of the core are well constrained by the application of liquid-state theory to seismic and laboratory data.
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                Author and article information

                Journal
                Earth and Planetary Science Letters
                Earth and Planetary Science Letters
                Elsevier BV
                0012821X
                July 2005
                July 2005
                : 236
                : 1-2
                : 78-95
                Article
                10.1016/j.epsl.2005.05.017
                3c5a6c83-7767-49b9-8cd1-8d8e88684bbd
                © 2005

                http://www.elsevier.com/tdm/userlicense/1.0/

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