Analytical study of the swing-by maneuver in an elliptical system
Autor(a) principal: | |
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Data de Publicação: | 2018 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1007/s10509-017-3242-5 http://hdl.handle.net/11449/179496 |
Resumo: | The objective of the present paper is to derive a set of analytical equations that describe a swing-by maneuver realized in a system of primaries that are in elliptical orbits. The goal is to calculate the variations of energy, velocity and angular momentum as a function of the usual basic parameters that describe the swing-by maneuver, as done before for the case of circular orbits. In elliptical orbits the velocity of the secondary body is no longer constant, as in the circular case, but it varies with the position of the secondary body in its orbit. As a consequence, the variations of energy, velocity and angular momentum become functions of the magnitude and the angle between the velocity vector of the secondary body and the line connecting the primaries. The “patched-conics” approach is used to obtain these equations. The configurations that result in maximum gains and losses of energy for the spacecraft are shown next, and a comparison between the results obtained using the analytical equations and numerical simulations are made to validate the method developed here. |
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Analytical study of the swing-by maneuver in an elliptical systemAstrodynamicsElliptical systemsSpacecraft trajectoriesSwing-by maneuversThe objective of the present paper is to derive a set of analytical equations that describe a swing-by maneuver realized in a system of primaries that are in elliptical orbits. The goal is to calculate the variations of energy, velocity and angular momentum as a function of the usual basic parameters that describe the swing-by maneuver, as done before for the case of circular orbits. In elliptical orbits the velocity of the secondary body is no longer constant, as in the circular case, but it varies with the position of the secondary body in its orbit. As a consequence, the variations of energy, velocity and angular momentum become functions of the magnitude and the angle between the velocity vector of the secondary body and the line connecting the primaries. The “patched-conics” approach is used to obtain these equations. The configurations that result in maximum gains and losses of energy for the spacecraft are shown next, and a comparison between the results obtained using the analytical equations and numerical simulations are made to validate the method developed here.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Instituto Nacional de Pesquisas Espaciais – INPEGrupo de Dinâmica Orbital e Planetologia Univ. Estadual Paulista – UNESPUniv. Estadual Paulista – UNESPGrupo de Dinâmica Orbital e Planetologia Univ. Estadual Paulista – UNESPUniv. Estadual Paulista – UNESPFAPESP: 2016/14665-2FAPESP: 2016/24561-0FAPESP: 2017/04643-4CNPq: 301338/2016-7CNPq: 312813/2013-9CNPq: 406841/2016-0Instituto Nacional de Pesquisas Espaciais – INPEUniversidade Estadual Paulista (Unesp)Ferreira, Alessandra F. S.Prado, Antônio F. B. A.Winter, Othon C. [UNESP]Santos, Denilson P. S. [UNESP]2018-12-11T17:35:25Z2018-12-11T17:35:25Z2018-02-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1007/s10509-017-3242-5Astrophysics and Space Science, v. 363, n. 2, 2018.1572-946X0004-640Xhttp://hdl.handle.net/11449/17949610.1007/s10509-017-3242-52-s2.0-850401024622-s2.0-85040102462.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstrophysics and Space Scienceinfo:eu-repo/semantics/openAccess2024-07-02T14:28:51Zoai:repositorio.unesp.br:11449/179496Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:31:36.602778Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Analytical study of the swing-by maneuver in an elliptical system |
title |
Analytical study of the swing-by maneuver in an elliptical system |
spellingShingle |
Analytical study of the swing-by maneuver in an elliptical system Ferreira, Alessandra F. S. Astrodynamics Elliptical systems Spacecraft trajectories Swing-by maneuvers |
title_short |
Analytical study of the swing-by maneuver in an elliptical system |
title_full |
Analytical study of the swing-by maneuver in an elliptical system |
title_fullStr |
Analytical study of the swing-by maneuver in an elliptical system |
title_full_unstemmed |
Analytical study of the swing-by maneuver in an elliptical system |
title_sort |
Analytical study of the swing-by maneuver in an elliptical system |
author |
Ferreira, Alessandra F. S. |
author_facet |
Ferreira, Alessandra F. S. Prado, Antônio F. B. A. Winter, Othon C. [UNESP] Santos, Denilson P. S. [UNESP] |
author_role |
author |
author2 |
Prado, Antônio F. B. A. Winter, Othon C. [UNESP] Santos, Denilson P. S. [UNESP] |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
Instituto Nacional de Pesquisas Espaciais – INPE Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Ferreira, Alessandra F. S. Prado, Antônio F. B. A. Winter, Othon C. [UNESP] Santos, Denilson P. S. [UNESP] |
dc.subject.por.fl_str_mv |
Astrodynamics Elliptical systems Spacecraft trajectories Swing-by maneuvers |
topic |
Astrodynamics Elliptical systems Spacecraft trajectories Swing-by maneuvers |
description |
The objective of the present paper is to derive a set of analytical equations that describe a swing-by maneuver realized in a system of primaries that are in elliptical orbits. The goal is to calculate the variations of energy, velocity and angular momentum as a function of the usual basic parameters that describe the swing-by maneuver, as done before for the case of circular orbits. In elliptical orbits the velocity of the secondary body is no longer constant, as in the circular case, but it varies with the position of the secondary body in its orbit. As a consequence, the variations of energy, velocity and angular momentum become functions of the magnitude and the angle between the velocity vector of the secondary body and the line connecting the primaries. The “patched-conics” approach is used to obtain these equations. The configurations that result in maximum gains and losses of energy for the spacecraft are shown next, and a comparison between the results obtained using the analytical equations and numerical simulations are made to validate the method developed here. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-12-11T17:35:25Z 2018-12-11T17:35:25Z 2018-02-01 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1007/s10509-017-3242-5 Astrophysics and Space Science, v. 363, n. 2, 2018. 1572-946X 0004-640X http://hdl.handle.net/11449/179496 10.1007/s10509-017-3242-5 2-s2.0-85040102462 2-s2.0-85040102462.pdf |
url |
http://dx.doi.org/10.1007/s10509-017-3242-5 http://hdl.handle.net/11449/179496 |
identifier_str_mv |
Astrophysics and Space Science, v. 363, n. 2, 2018. 1572-946X 0004-640X 10.1007/s10509-017-3242-5 2-s2.0-85040102462 2-s2.0-85040102462.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Astrophysics and Space Science |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
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1808128373801615360 |