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• W2801549162 abstract "Significance During accretion, giant impacts may partially vaporize planets, with profound consequences for energy and mass transfer between the growing planet and its satellites. We find that giant impacts produce much more supercritical fluid than previously thought, with a much lower liquid–vapor critical temperature. The vapor is depleted in Mg with respect to coexisting liquid and has very different chemical bonding, being dominated by covalent molecules (O 2 and SiO) up to the critical point. These molecules also appear in significant fractions within the near-critical liquid phase, making the liquid structure fundamentally different from that near the melting point." @default.
• W2801549162 created "2018-05-17" @default.
• W2801549162 creator A5055320146 @default.
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• W2801549162 date "2018-05-07" @default.
• W2801549162 modified "2023-09-25" @default.
• W2801549162 title "Critical vaporization of MgSiO ₃" @default.
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• W2801549162 doi "https://doi.org/10.1073/pnas.1719134115" @default.
• W2801549162 hasPubMedCentralId "https://www.ncbi.nlm.nih.gov/pmc/articles/6003494" @default.
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