@InProceedings{FormigaPrad:2011:OrChDu,
author = "Formiga, J. K. S. and Prado, A. F. B. A.",
affiliation = "{Technology Faculty-FATEC-SJC} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Orbital Characteristics Due to the Three Dimensional Swing-By in
the Sun-Jupiter System",
booktitle = "Proceedings...",
year = "2011",
pages = "61--69",
organization = "10. International Conference on Computational Intelligence
Man-Machine Systems and Cybernetics",
publisher = "he World Scientific and Engineering Academy and Society Press",
keywords = "orbital maneuver, three dimensional swing-by, celestial mechanics,
orbital dynamics.",
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.",
conference-location = "Jakarta",
conference-year = "2011",
isbn = "978-1-61804-049-7",
language = "en",
targetfile = "CIMISP-09.pdf",
volume = "1",
urlaccessdate = "15 jan. 2021"
}