Traveling between the Earth-Moon Lagrangian points and the earth

Detalhes bibliográficos
Autor(a) principal: Oliveira, Geraldo Magela Couto
Data de Publicação: 2016
Outros Autores: Prado, Antonio Fernando Bertachini de Almeida, Sanchez, Diogo Merguizo, Gomes, Vivian Martins [UNESP]
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://hdl.handle.net/11449/178183
Resumo: The idea of the present paper is to study orbital transfers for a spacecraft from the Lagrangian points in the Earth-Moon system to the Earth, as well as to the other Lagrangian points. The model used is the restricted three-body problem with the addition of the effects of the radiation pressure in the trajectory of the spacecraft. The basic maneuver is a bi-impulsive transfers under the dynamics explained before. The results show that the radiation pressure has an influence in the process, although not very large. After that we made some simulations for similar maneuvers in a double asteroid system, where the gravitational forces are smaller and the radiation pressure gives important contributions to the motion of the spacecraft. It is possible to find solutions with smaller fuel consumption when considering the solar radiation pressure, in both cases, but with important reductions in the magnitude of the impulses required for the asteroid system. It is important always to take into account that the idea presented here is not to use the radiation pressure as a control, but just to measure its effects when performing the bi-impulsive transfer.
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spelling Traveling between the Earth-Moon Lagrangian points and the earthThe idea of the present paper is to study orbital transfers for a spacecraft from the Lagrangian points in the Earth-Moon system to the Earth, as well as to the other Lagrangian points. The model used is the restricted three-body problem with the addition of the effects of the radiation pressure in the trajectory of the spacecraft. The basic maneuver is a bi-impulsive transfers under the dynamics explained before. The results show that the radiation pressure has an influence in the process, although not very large. After that we made some simulations for similar maneuvers in a double asteroid system, where the gravitational forces are smaller and the radiation pressure gives important contributions to the motion of the spacecraft. It is possible to find solutions with smaller fuel consumption when considering the solar radiation pressure, in both cases, but with important reductions in the magnitude of the impulses required for the asteroid system. It is important always to take into account that the idea presented here is not to use the radiation pressure as a control, but just to measure its effects when performing the bi-impulsive transfer.Federal Center for Technological Education of Minas Gerais CEFET-MGNational Institute for Space Research INPESão Paulo State University FEG/UNESPSchool of Aeronautics and Astronautics Purdue University, 701 West Stadium AvenueSão Paulo State University FEG UNESPSão Paulo State University FEG/UNESPSão Paulo State University FEG UNESPCEFET-MGINPEUniversidade Estadual Paulista (Unesp)Purdue UniversityOliveira, Geraldo Magela CoutoPrado, Antonio Fernando Bertachini de AlmeidaSanchez, Diogo MerguizoGomes, Vivian Martins [UNESP]2018-12-11T17:29:11Z2018-12-11T17:29:11Z2016-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject14th International Conference on Space Operations, 2016.http://hdl.handle.net/11449/1781832-s2.0-84980038903Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPeng14th International Conference on Space Operations, 2016info:eu-repo/semantics/openAccess2021-10-23T21:47:04Zoai:repositorio.unesp.br:11449/178183Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462021-10-23T21:47:04Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Traveling between the Earth-Moon Lagrangian points and the earth
title Traveling between the Earth-Moon Lagrangian points and the earth
spellingShingle Traveling between the Earth-Moon Lagrangian points and the earth
Oliveira, Geraldo Magela Couto
title_short Traveling between the Earth-Moon Lagrangian points and the earth
title_full Traveling between the Earth-Moon Lagrangian points and the earth
title_fullStr Traveling between the Earth-Moon Lagrangian points and the earth
title_full_unstemmed Traveling between the Earth-Moon Lagrangian points and the earth
title_sort Traveling between the Earth-Moon Lagrangian points and the earth
author Oliveira, Geraldo Magela Couto
author_facet Oliveira, Geraldo Magela Couto
Prado, Antonio Fernando Bertachini de Almeida
Sanchez, Diogo Merguizo
Gomes, Vivian Martins [UNESP]
author_role author
author2 Prado, Antonio Fernando Bertachini de Almeida
Sanchez, Diogo Merguizo
Gomes, Vivian Martins [UNESP]
author2_role author
author
author
dc.contributor.none.fl_str_mv CEFET-MG
INPE
Universidade Estadual Paulista (Unesp)
Purdue University
dc.contributor.author.fl_str_mv Oliveira, Geraldo Magela Couto
Prado, Antonio Fernando Bertachini de Almeida
Sanchez, Diogo Merguizo
Gomes, Vivian Martins [UNESP]
description The idea of the present paper is to study orbital transfers for a spacecraft from the Lagrangian points in the Earth-Moon system to the Earth, as well as to the other Lagrangian points. The model used is the restricted three-body problem with the addition of the effects of the radiation pressure in the trajectory of the spacecraft. The basic maneuver is a bi-impulsive transfers under the dynamics explained before. The results show that the radiation pressure has an influence in the process, although not very large. After that we made some simulations for similar maneuvers in a double asteroid system, where the gravitational forces are smaller and the radiation pressure gives important contributions to the motion of the spacecraft. It is possible to find solutions with smaller fuel consumption when considering the solar radiation pressure, in both cases, but with important reductions in the magnitude of the impulses required for the asteroid system. It is important always to take into account that the idea presented here is not to use the radiation pressure as a control, but just to measure its effects when performing the bi-impulsive transfer.
publishDate 2016
dc.date.none.fl_str_mv 2016-01-01
2018-12-11T17:29:11Z
2018-12-11T17:29:11Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
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dc.identifier.uri.fl_str_mv 14th International Conference on Space Operations, 2016.
http://hdl.handle.net/11449/178183
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identifier_str_mv 14th International Conference on Space Operations, 2016.
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url http://hdl.handle.net/11449/178183
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 14th International Conference on Space Operations, 2016
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reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
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