Publication Date:
2019-06-28
Description:
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.
Keywords:
LUNAR AND PLANETARY EXPLORATION
Type:
NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986; p 141-143
Format:
application/pdf