On the original distribution of the asteroids. II - Do stable orbits exist between Jupiter and Saturn?

Computer Science

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Asteroids, Eccentric Orbits, Orbital Mechanics, Solar Orbits, Spatial Distribution, Chaos, Cosmology, Interplanetary Space, Jupiter (Planet), Planetary Evolution, Saturn (Planet), Asteroids, Distribution, Orbits, Stability, Gravity Effects, Jupiter, Perturbations, Saturn, Distance, Orbital Elements, Eccentricity, Models, Computer Methods, Ejection

Scientific paper

Prompted by the recent indication by Wisdom (1987) that orbits may appear stable for very long periods and then suddenly become chaotic, an earlier integration of asteroidlike orbits between Jupiter and Saturn in which most of the asteroids had close encounters with these planets and were removed is extended nearly 2000 times longer. Where two bands, centered on 1.35 and 1.45 Jovian distances, harbored asteroids before, all the asteroids are presently removed. Asteroids are found to be removed by Saturn-orbit crossings 5 times more frequently than by Jupiter-orbit crossing.

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