Powered swing-by maneuvers around the Moon

Detalhes bibliográficos
Autor(a) principal: Silva, A. F.
Data de Publicação: 2013
Outros Autores: Prado, A. F.B.A., Winter, O. C. [UNESP]
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1742-6596/465/1/012001
http://hdl.handle.net/11449/232191
Resumo: A Swing-By maneuver occurs when a satellite approaches a celestial body to gain or lose energy from its gravitational field. The present work studies Swing-By maneuvers that are combined with the use of an impulsive thrust in different directions during the passage of the spacecraft by the periapsis of its trajectory around the Moon. The main objective of this type of maneuver is the fuel economy for orbital transfers. From the results, it is visible that the best direction to apply the impulse is not the direction to the motion of the spacecraft, as might be expected. In fact, by using a different direction, it is possible to maximize the effects of the Swing-By by decreasing the periapsis distance and/or increasing the turning angle of the maneuver, that are the key parameters to specify the variation of energy due to the Swing-By. The changes in the periapsis distance and turning angle cause modifications in the geometry of the original Swing-By, generating a maneuver with new parameters. This new Swing-By compensates for the loss of energy transfer that results of applying the impulse in a in a non-tangential direction.
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spelling Powered swing-by maneuvers around the MoonA Swing-By maneuver occurs when a satellite approaches a celestial body to gain or lose energy from its gravitational field. The present work studies Swing-By maneuvers that are combined with the use of an impulsive thrust in different directions during the passage of the spacecraft by the periapsis of its trajectory around the Moon. The main objective of this type of maneuver is the fuel economy for orbital transfers. From the results, it is visible that the best direction to apply the impulse is not the direction to the motion of the spacecraft, as might be expected. In fact, by using a different direction, it is possible to maximize the effects of the Swing-By by decreasing the periapsis distance and/or increasing the turning angle of the maneuver, that are the key parameters to specify the variation of energy due to the Swing-By. The changes in the periapsis distance and turning angle cause modifications in the geometry of the original Swing-By, generating a maneuver with new parameters. This new Swing-By compensates for the loss of energy transfer that results of applying the impulse in a in a non-tangential direction.Instituto Nacional de Pesquisas Espaciais INPE, São José dos CamposGrupo de Dinâmica Orbital and Planetologia University Estadual Paulista UNESP, GuaratinguetáGrupo de Dinâmica Orbital and Planetologia University Estadual Paulista UNESP, GuaratinguetáINPEUniversidade Estadual Paulista (UNESP)Silva, A. F.Prado, A. F.B.A.Winter, O. C. [UNESP]2022-04-29T09:12:17Z2022-04-29T09:12:17Z2013-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjecthttp://dx.doi.org/10.1088/1742-6596/465/1/012001Journal of Physics: Conference Series, v. 465, n. 1, 2013.1742-65961742-6588http://hdl.handle.net/11449/23219110.1088/1742-6596/465/1/0120012-s2.0-84890631616Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of Physics: Conference Seriesinfo:eu-repo/semantics/openAccess2024-07-02T14:29:48Zoai:repositorio.unesp.br:11449/232191Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:20:22.795718Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Powered swing-by maneuvers around the Moon
title Powered swing-by maneuvers around the Moon
spellingShingle Powered swing-by maneuvers around the Moon
Silva, A. F.
title_short Powered swing-by maneuvers around the Moon
title_full Powered swing-by maneuvers around the Moon
title_fullStr Powered swing-by maneuvers around the Moon
title_full_unstemmed Powered swing-by maneuvers around the Moon
title_sort Powered swing-by maneuvers around the Moon
author Silva, A. F.
author_facet Silva, A. F.
Prado, A. F.B.A.
Winter, O. C. [UNESP]
author_role author
author2 Prado, A. F.B.A.
Winter, O. C. [UNESP]
author2_role author
author
dc.contributor.none.fl_str_mv INPE
Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Silva, A. F.
Prado, A. F.B.A.
Winter, O. C. [UNESP]
description A Swing-By maneuver occurs when a satellite approaches a celestial body to gain or lose energy from its gravitational field. The present work studies Swing-By maneuvers that are combined with the use of an impulsive thrust in different directions during the passage of the spacecraft by the periapsis of its trajectory around the Moon. The main objective of this type of maneuver is the fuel economy for orbital transfers. From the results, it is visible that the best direction to apply the impulse is not the direction to the motion of the spacecraft, as might be expected. In fact, by using a different direction, it is possible to maximize the effects of the Swing-By by decreasing the periapsis distance and/or increasing the turning angle of the maneuver, that are the key parameters to specify the variation of energy due to the Swing-By. The changes in the periapsis distance and turning angle cause modifications in the geometry of the original Swing-By, generating a maneuver with new parameters. This new Swing-By compensates for the loss of energy transfer that results of applying the impulse in a in a non-tangential direction.
publishDate 2013
dc.date.none.fl_str_mv 2013-01-01
2022-04-29T09:12:17Z
2022-04-29T09:12:17Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/conferenceObject
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status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1088/1742-6596/465/1/012001
Journal of Physics: Conference Series, v. 465, n. 1, 2013.
1742-6596
1742-6588
http://hdl.handle.net/11449/232191
10.1088/1742-6596/465/1/012001
2-s2.0-84890631616
url http://dx.doi.org/10.1088/1742-6596/465/1/012001
http://hdl.handle.net/11449/232191
identifier_str_mv Journal of Physics: Conference Series, v. 465, n. 1, 2013.
1742-6596
1742-6588
10.1088/1742-6596/465/1/012001
2-s2.0-84890631616
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of Physics: Conference Series
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eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
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repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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