Formation of terrestrial planets in a dissipating gas disk with Jupiter and Saturn
- 29 November 2003
- Vol. 167 (2) , 231-243
- https://doi.org/10.1016/j.icarus.2003.10.005
Abstract
No abstract availableKeywords
This publication has 25 references indexed in Scilit:
- The effects of nebula surface density profile and giant‐planet eccentricities on planetary accretion in the inner solar systemMeteoritics & Planetary Science, 2002
- Damping of Terrestrial‐Planet Eccentricities by Density‐Wave Interactions with a Remnant Gas DiskThe Astrophysical Journal, 2002
- The Gas-Drag Effect on the Orbital Instability of a Protoplanet SystemPublications of the Astronomical Society of Japan, 2001
- Planets in the asteroid beltMeteoritics & Planetary Science, 2001
- On the Character and Consequences of Large Impacts in the Late Stage of Terrestrial Planet FormationIcarus, 1999
- Stability and Instability of the Terrestrial Protoplanet System and Their Possible Roles in the Final Stage of Planet FormationIcarus, 1999
- Making the Terrestrial Planets: N-Body Integrations of Planetary Embryos in Three DimensionsIcarus, 1998
- The Stability of Multi-Planet SystemsIcarus, 1996
- Disk-Satellite Interaction via Density Waves and the Eccentricity Evolution of Bodies Embedded in DisksThe Astrophysical Journal, 1993
- 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