Equation of state experiments and theory relevant to planetary modelling

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Models, Galilean Satellites, Hugoniot Equation Of State, Mathematical Models, Planetary Composition, Pressure Measurement, Compression Waves, Gas Pressure, Helium, Hydrogen, Iron, Planetary Structure, Shock Waves, Thermodynamics, Planets, Models, Equations Of State, Theoretical Studies, Experiments, Shock Effects, Compression, Pressure, Parameters, Diagrams, Hydrogen, Helium, Iron, Giant Planets, Thermodynamics, Cores, Jupiter, Saturn, Uranus, Neptune, Electrical Properties, Conductivity, Immis

Scientific paper

In recent years there have been a number of static and shockwave experiments on the properties of planetary materials. The highest pressure measurements, and the ones most relevant to planetary modelling, have been obtained by shock compression. Of particular interest to the Jovian group are results for H2, H2O, CH4 and NH3. Although the properties of metallic hydrogen have not been measured, they have been the subject of extensive calculations. In addition recent shock wave experiments on iron report to have detected melting under earth core conditions. From this data theoretical models have been developed for computing the equations of state of materials used in planetary studies. A compelling feature that has followed from the use of improved material properties is a simplification in the planetary models.

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