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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Study of the gravitational capture of a spacecraft by Jupiter

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Author(s):
Brasil, P. I. O. ; Prado, A. F. B. A. ; Deienno, R. ; Yokoyama, T.
Total Authors: 4
Document type: Journal article
Source: Advances in Space Research; v. 55, n. 2, p. 668-681, JAN 15 2015.
Web of Science Citations: 7
Abstract

An extensive analysis of the gravitational capture of a spacecraft by Jupiter is performed for the main regions of interest around this planet. Four different dynamical models are used to study the problem. Our methodology is analogous to the one used to study the gravitational capture maneuvers in the Earth-Moon system. However, here the motion of the spacecraft is free to occupy the three-dimensional space rather than been limited to the orbital plane of the primaries, that is the most usual approach available in the literature. Similarly to what was done in the Earth-Moon system, the two-body energy Jupiter-spacecraft is monitored all the time and an impulsive maneuver should be applied to complete the capture when the spacecraft reaches the periapsis of the close approach trajectory. Our results show that the presence of the oblateness of Jupiter in the dynamical model is essential to obtain lower values for the two-body energy in times that are not too long for practical missions. The Galilean satellites are also very important, and despite their contribution in the gravitational capture maneuver itself, they can be used as a source of swing-bys that decrease the two-body energy Jupiter-spacecraft. (C) 2014 COSPAR. Published by Elsevier Ltd. All rights reserved. (AU)

FAPESP's process: 10/11109-5 - Satellites of Saturn: Stability, Capture and Analysis of the Excitations on the Eccentricity and Inclination of the Regular Satellites During the Planetary Migration
Grantee:Rogerio Deienno
Support Opportunities: Scholarships in Brazil - Doctorate
FAPESP's process: 11/08540-9 - Dynamical formation of trans-Neptunian detached objects near mean motion resonances with Neptune
Grantee:Pedro Ivo de Oliveira Brasil
Support Opportunities: Scholarships in Brazil - Doctorate