On the origin of the planetary spin by accretion of planetesimals: II. Collisional orbits at the hill surface
- 30 November 1991
- journal article
- Published by Elsevier BV in Icarus
- Vol. 94 (1), 112-125
- https://doi.org/10.1016/0019-1035(91)90144-i
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Did rotation of the protoplanets originate from the successive collisions of planetesimals?Icarus, 1990
- The fractal dynamics of satellite capture in the circular restricted three-body problemThe Astronomical Journal, 1989
- On the origin of the planetary spin angular momentum by accretion of planetesimals: Property of collision orbitsIcarus, 1989
- Outcomes of planetary close encounters: A systematic comparison of methodologiesIcarus, 1988
- Satellite encountersIcarus, 1986
- Series expansions for encounter-type solutions of Hill's problemCelestial Mechanics and Dynamical Astronomy, 1986
- The range of validity of the two-body approximation in models of terrestrial planet accumulation: II. Gravitational cross sections and runaway accretionIcarus, 1985
- Collisional Processes of Planetesimals with a Protoplanet under the Gravity of the Proto-SunProgress of Theoretical Physics, 1983
- Impossibility of the capture of retrograde satellites in the restricted three-body problemCelestial Mechanics and Dynamical Astronomy, 1983
- On the rotation of the Earth produced by gravitational accretion of particlesIcarus, 1968