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• W1539041623 abstract "The physical mechanisms driving thermal and chemical evolution of large icy satellites depend on the thermodynamic properties of the high pressure phases of ice. After reviewing some important aspects of the internal dynamics of the large icy satellites of Jupiter and Saturn, this paper describes the phase diagram of water ice and its variations due to the presence of other chemical compounds. Values of the elastic parameters and other thermodynamic constants are given. To illustrate how the experimental data strongly influence models of the internal structure and evolution of icy satellites, the effect of ammonia on the internal structure of Europa and Titan is described." @default.
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• W1539041623 date "1998-01-01" @default.
• W1539041623 modified "2023-10-14" @default.
• W1539041623 title "Thermodynamic Properties of High Pressure Ices: Implications for the Dynamics and Internal Structure of Large Icy Satellites" @default.
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• W1539041623 doi "https://doi.org/10.1007/978-94-011-5252-5_4" @default.
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