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Orbits of Trojan Asteroids
Published online by Cambridge University Press: 14 August 2015
Abstract
In this paper the orbital evolution of Trojan asteroids are studied by integrating numerically the equations of motion over the interval 1660–2060, perturbations from Venus to Pluto being taken into account. The comparison of the actual motion of Trojans in the solar system with the theory based on the restricted three-body problem are given.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 62: The Stability of the Solar System , 1974 , pp. 63 - 69
- Copyright
- Copyright © Reidel 1974
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