The role of secular resonances on trojans of the terrestrial planets
- 21 July 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 334 (1) , 241-247
- https://doi.org/10.1046/j.1365-8711.2002.05526.x
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Asteroids in the inner Solar system - I. ExistenceMonthly Notices of the Royal Astronomical Society, 2002
- Hamiltonian formulation of the secular theory for Trojan-type motionAstronomy & Astrophysics, 2001
- The effect of eccentricity and inclination on the motion near the Lagrangian points L4 and L5Celestial Mechanics and Dynamical Astronomy, 2000
- The Trojan problemCelestial Mechanics and Dynamical Astronomy, 1997
- On the stability of high inclination TrojansEarth, Moon, and Planets, 1995
- On the stability of Martian TrojansThe Astronomical Journal, 1994
- A preliminary analysis of the orbit of the Mars Trojan asteroid (5261) EurekaCelestial Mechanics and Dynamical Astronomy, 1994
- The chaotic motion of the solar system: A numerical estimate of the size of the chaotic zonesIcarus, 1990
- Studies on solar system dynamics. II - The stability of earth's TrojansThe Astronomical Journal, 1990
- Secular perturbations of asteroids with high inclination and eccentricityThe Astronomical Journal, 1962