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. 15 refs., 2 figs
Hydrogen and helium are the major constituents of Jupiter and Saturn, and phase transitions can have...
Structure models of the interior of gas and ice giants are designed to fit available observational c...
This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Planetary...
Models of Jupiter and Saturn postulate a central rock core surrounded by a fluid mixture of hydrogen...
128 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2009.We also study the equation of...
We examine the comparative thermal evolution of Jupiter and Saturn, applying recent theoretical resu...
In this work, the miscibility gap of hydrogen-helium mixtures is calculated under conditions relevan...
An experimental observation that requires a theoretical explanation is the large excess energy radia...
We build on recent new evolutionary models of Jupiter and Saturn and here extend our calculations to...
A new approach is developed for evaluating the mixing properties of binary solutions at high pressur...
The free energy of a hydrogen-helium fluid mixture is evaluated for the temperatures and densities a...
The free energy of a hydrogen-helium fluid mixture is evaluated for the temperatures and densities a...
Understanding the interior of Jupiter depends upon our knowledge of the thermodynamics and transpor...
Supplemental materials of Howard & Guillot (2023, A&A). Abstract: Context. The equation of state f...
We present evolutionary sequences for Jupiter and Saturn, based on new nongray model atmospheres, wh...
Hydrogen and helium are the major constituents of Jupiter and Saturn, and phase transitions can have...
Structure models of the interior of gas and ice giants are designed to fit available observational c...
This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Planetary...
Models of Jupiter and Saturn postulate a central rock core surrounded by a fluid mixture of hydrogen...
128 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2009.We also study the equation of...
We examine the comparative thermal evolution of Jupiter and Saturn, applying recent theoretical resu...
In this work, the miscibility gap of hydrogen-helium mixtures is calculated under conditions relevan...
An experimental observation that requires a theoretical explanation is the large excess energy radia...
We build on recent new evolutionary models of Jupiter and Saturn and here extend our calculations to...
A new approach is developed for evaluating the mixing properties of binary solutions at high pressur...
The free energy of a hydrogen-helium fluid mixture is evaluated for the temperatures and densities a...
The free energy of a hydrogen-helium fluid mixture is evaluated for the temperatures and densities a...
Understanding the interior of Jupiter depends upon our knowledge of the thermodynamics and transpor...
Supplemental materials of Howard & Guillot (2023, A&A). Abstract: Context. The equation of state f...
We present evolutionary sequences for Jupiter and Saturn, based on new nongray model atmospheres, wh...
Hydrogen and helium are the major constituents of Jupiter and Saturn, and phase transitions can have...
Structure models of the interior of gas and ice giants are designed to fit available observational c...
This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Planetary...