The solubility of oxygen in molten iron increases at high temperature. Could this explain why Earth's mantle is poor in iron oxide, whereas the mantle of Mars, which formed under cooler conditions, is not?
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References
Birch, F. J. Geophys. Res. 69, 4377–4388 (1964).
Kato, T. & Ringwood, A. E. Phys. Chem. Miner. 16, 524–538 (1989).
Rubie, D. C., Gessmann, C. K. & Frost, D. J. Nature 429, 58–61 (2004).
Li, J. & Agee, C. B. Geophys. Res. Lett. 28, 81–84 (2001).
O'Neill, H. S. C., Canil, D. & Rubie, D. C. J. Geophys. Res. 103, 12239–12260 (1998).
Li, J. & Agee, C. B. Nature 381, 686–689 (1996).
Chabot, N. L. & Agee, C. B. Geochim. Cosmochim. Acta 67, 2077–2091 (2003).
Dreibus, G. & Wänke, H. Hans Suess Festschrift 20, 367–381 (1985).
Folkner, W. M. et al. Science 278, 1749–1751 (1997).
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Agee, C. Hot metal. Nature 429, 33–34 (2004). https://doi.org/10.1038/429033a
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DOI: https://doi.org/10.1038/429033a