Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jass....5..129p&link_type=abstract
Journal of Astronomy and Space Science, vol. 5, no. 2, p. 129-141.
Astronomy and Astrophysics
Astronomy
Scientific paper
Using the numerical solution in the plane restricted problem of three bodies, about 490 periodic orbits are computed numerically around the L5 of Sun-Jupiter and about 1600 periodic orbits also be done around the L5 of Earth-Moon system. As period increase, the energy and the shape of periodic orbits increase around the L5 of Sun-Jupiter system. But, in Earth-Moon system, the complex shapes and dents appear around the L5 and periodic orbits intersect one another in the place where dents are shown. And there is a region that three different periodic orbits exist with the same period in this region. The regions can exist around the L5 of Sun-Jupiter system where periodic orbit can be unstable by perturbation of other force besides the gravitational force of Jupiter. These regions which is close to L5 are a ¡ 5.29 AU. The Trojan asteroids that have a small eccentricity and inclination can not exist in this region.
Choi Kyu-Hong
Jo Jung-Hyun
Lee Byoung-Sun
Park Sang-Young
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