The three principal secular resonances ?5, ?6, and ?16 in the asteroidal belt
- 1 January 1989
- journal article
- Published by Springer Nature in Celestial Mechanics and Dynamical Astronomy
- Vol. 46 (3) , 231-251
- https://doi.org/10.1007/bf00049260
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Dynamical relations between asteroids, meteorites and Apollo-Amor objectsPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1987
- A simple analytical model for the secular resonance ?6 in the asteroidal beltCelestial Mechanics and Dynamical Astronomy, 1987
- Secular resonances: New resultsCelestial Mechanics and Dynamical Astronomy, 1987
- Secular perturbations of asteroids in secular resonanceCelestial Mechanics and Dynamical Astronomy, 1985
- Trojan orbits in secular resonancesCelestial Mechanics and Dynamical Astronomy, 1984
- Chaotic behavior and the origin of the 31 Kirkwood gapIcarus, 1983
- The positions of secular resonance surfacesIcarus, 1981
- Notes on the origin of the Trojan asteroidsIcarus, 1979
- Steady state populations of Apollo-Amor objectsIcarus, 1979
- Secular resonance, solar spin down, and the orbit of MercuryIcarus, 1976