Other
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...83..382w&link_type=abstract
Icarus (ISSN 0019-1035), vol. 83, Feb. 1990, p. 382-390. Research supported by NSF.
Other
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Dynamic Characteristics, Jupiter (Planet), Saturn (Planet), Solar Orbits, Planetary Mass, Solar System, Asteroids, Orbits, Stability, Computer Methods, Timescale, Solar System, Eccentricity, Orbital Elements, Inclination, Gravity Effects, Jupiter, Saturn, Particles, Ejection, Planet Crossers, Simulations, Procedure, Perturbations, Celestial Mechanics, Trojan Asteroids, Lagrange Points
Scientific paper
The present experiment with test particles placed in orbits at uniform intervals between 5.7 and 8.8 AU, with randomly distributed eccentricities between 0.0 and 0.02 and inclinations between 0.0 and 0.063 rad, leads to the perception that no stable niches exist in the Jupiter-Saturn zone other than the Lagrangian points of Jupiter. These points are populated by at least 26 Trojan asteroids. The primary implication of these results for future investigations of the Saturn-Uranus-Neptune zone is that experimental design should be as selective as the dynamics of the planetary system have been shown to be.
Kaula William M.
Newman William I.
Weibel W. M.
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