From planetesimals to terrestrial planets: N-body simulations including the effects of nebular gas and giant planets
- 30 June 2010
- journal article
- Published by Elsevier BV in Icarus
- Vol. 207 (2), 517-535
- https://doi.org/10.1016/j.icarus.2009.11.038
Abstract
No abstract availableKeywords
This publication has 79 references indexed in Scilit:
- THE TWO MODES OF GAS GIANT PLANET FORMATIONThe Astrophysical Journal, 2009
- Planetesimal formation near the snow line in MRI-driven turbulent protoplanetary disksAstronomy & Astrophysics, 2008
- The major differentiation of the Earth at ∼4.45 GaEarth and Planetary Science Letters, 2008
- On the Corotation Torque in a Radiatively Inefficient DiskThe Astrophysical Journal, 2008
- Hit-and-run planetary collisionsNature, 2006
- Accretion Efficiency during Planetary CollisionsThe Astrophysical Journal, 2004
- Damping of Terrestrial‐Planet Eccentricities by Density‐Wave Interactions with a Remnant Gas DiskThe Astrophysical Journal, 2002
- On the Character and Consequences of Large Impacts in the Late Stage of Terrestrial Planet FormationIcarus, 1999
- Calculations of the accretion and evolution of giant planets: The effects of solid coresIcarus, 1986
- The Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar NebulaProgress of Theoretical Physics, 1976