Stirring and dynamical friction rates of planetesimals in the solar gravitational field
- 1 November 1990
- Vol. 88 (1), 129-145
- https://doi.org/10.1016/0019-1035(90)90182-9
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Runaway planetary growth with collision rate in the solar gravitational fieldIcarus, 1990
- Stirring of a planetesimal swarm: The role of distant encountersIcarus, 1989
- Accumulation of a swarm of small planetesimalsIcarus, 1989
- Evolution of planetesimal velocitiesIcarus, 1988
- Chapter 15. Hill's Approximation in the Three-Body ProblemProgress of Theoretical Physics Supplement, 1988
- The range of validity of the two-body approximation in models of terrestrial planet accumulation: I. Gravitational perturbationsIcarus, 1984
- Accumulation of planetesimals in the solar nebulaIcarus, 1983
- The Dynamics of Planetary RingsAnnual Review of Astronomy and Astrophysics, 1982
- Numerical experiment applicable to the latest stage of planet growthIcarus, 1982
- Structure of the Solar Nebula, Growth and Decay of Magnetic Fields and Effects of Magnetic and Turbulent Viscosities on the NebulaProgress of Theoretical Physics Supplement, 1981