Properties of planetary fluids at high pressure and temperature

Details Properties of planetary fluids at high pressure and temperature Properties of planetary fluids at high pressure and temperature

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pggp.rept..141n&link_type=abstract

In NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986 p 141-143 (SEE N87-23341 16-91)

Physics

Geophysics

High Pressure, High Temperature, Jupiter (Planet), Liquids, Neptune (Planet), Planetary Composition, Saturn (Planet), Uranus (Planet), Cooling, Electrical Resistivity, Equations Of State, Methane, Models, Nitrogen, Planetary Magnetic Fields, Planetary Rotation, Temperature Measurement

Scientific paper

In order to derive models of the interiors of Uranus, Neptune, Jupiter and Saturn, researchers studied equations of state and electrical conductivities of molecules at high dynamic pressures and temperatures. Results are given for shock temperature measurements of N2 and CH4. Temperature data allowed demonstration of shock induced cooling in the the transition region and the existence of crossing isotherms in P-V space.

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