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• W115389075 abstract "This paper presents an analytical and numerical study about orbital characteristics of trajectories due to a three dimensional swing-by maneuver between a planet and a particle. The model used has the same hypothesis of the circular restricted three-body problem. It is assumed that the forces are given by two main bodies that are in circular orbits around their center of mass and that the particles are moving under the gravitational attraction of these two primaries. This method has been under study for a long time by several authors, most of them used the dynamical system given by the patched-conics. The technique shown here generates accurate solutions for interplanetary transfer description. Two solutions are considered for the Swing-By (clock-wise and counter-clock-wise orbit). The goal is to study the orbital change due to the variation of inclination, longitude of the ascending node and argument of periapsis, considering two angles of approaches. Finally, numerical simulations are performed using the Sun-Jupiter system to determine the evolution of the cloud of particles during the maneuver and to map regions for optimal maneuvers." @default.
• W115389075 created "2016-06-24" @default.
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• W115389075 date "2011-12-01" @default.
• W115389075 modified "2023-09-23" @default.
• W115389075 title "Orbital characteristics due to the three dimensional swing-by in the Sun-Jupiter system" @default.
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