Hydrogen-Helium Mixtures at Megabar Pressures: Implications for Jupiter and Saturn
- 15 November 1991
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 254 (5034) , 986-989
- https://doi.org/10.1126/science.254.5034.986
Abstract
Models of Jupiter and Saturn postulate a central rock core surrounded by a fluid mixture of hydrogen and helium. These models suggest that the mixture is undergoing phase separation in Saturn but not Jupiter. State-of-the-art total energy calculations of the enthalpy of mixing for ordered alloys of hydrogen and helium confirm that at least partial phase separation has occurred in Saturn and predict that this process has also begun in Jupiter.Keywords
This publication has 21 references indexed in Scilit:
- Equation of state of the one-component plasma derived from precision Monte Carlo calculationsPhysical Review A, 1990
- Theory of high-pressure phases of hydrogenPhysical Review Letters, 1989
- Statistical mechanics of light elements at high pressure. VII - A perturbative free energy for arbitrary mixtures of H and HeThe Astrophysical Journal, 1985
- Statistical mechanics of light elements at high pressure. VI - Liquid-state calculations with Thomas-Fermi-Dirac theoryThe Astrophysical Journal, 1984
- Albedo, internal heat flux, and energy balance of SaturnIcarus, 1983
- Statistical mechanics of dense ionized matter. VII. Equation of state and phase separation of ionic mixtures in a uniform backgroundPhysical Review A, 1977
- Phase separation for a dense fluid mixture of nucleiPhysical Review A, 1977
- On Convection and Gravitational Layering in Jupiter and in Stars of Low MassThe Astrophysical Journal, 1973
- Internal Structure and Energy Emission of JupiterNature, 1967
- Electron Screening and Thermonuclear ReactionsAustralian Journal of Physics, 1954