Calculations of the accretion and evolution of giant planets: The effects of solid cores
- 1 September 1986
- Vol. 67 (3), 391-408
- https://doi.org/10.1016/0019-1035(86)90122-3
Abstract
No abstract availableKeywords
This publication has 31 references indexed in Scilit:
- Planetesimal dissolution in the envelopes of the forming, giant planetsIcarus, 1986
- The range of validity of the two-body approximation in models of terrestrial planet accumulation: II. Gravitational cross sections and runaway accretionIcarus, 1985
- Cosmochemistry and structure of the giant planets and their satellitesIcarus, 1985
- From icy planetesimals to outer planets and cometsIcarus, 1984
- Computation of Jupiter interior models from gravitational inversion theoryIcarus, 1983
- Accumulation of planetesimals in the solar nebulaIcarus, 1983
- On the evolution of convective accretion disk models of the primordial solar nebulaThe Astrophysical Journal, 1982
- Thermodynamics of dense hydrogen-helium fluidsThe Astrophysical Journal, 1975
- Hydrodynamic instability of the solar nebula in the presence of a planetary coreIcarus, 1974
- Internal Structure and Energy Emission of JupiterNature, 1967