Powered swing-by maneuvers around the Moon
Autor(a) principal: | |
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Data de Publicação: | 2013 |
Outros Autores: | , |
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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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 |
format |
conferenceObject |
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 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
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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1808129417001566208 |