Trojan capture by terrestrial planets

摘要: The paper is devoted to investigate the capture of asteroids by Venus, Earth and Mars into 1:1 mean-motion resonance, especially Trojan orbits. Current theoretical studies predict that are a frequent by-product planet formation. This not only case for outer giant planets, but also terrestrial planets in inner Solar System. By using numerical integrations, we investigated efficiency stability captured objects. We found out larger System compared ones, most long term stable. These temporary captures caused chaotic behaviour objects were without any dissipative forces. They show an interesting dynamical mixing, like jumping from one Lagrange point other one.