Controlling the eccentricity of polar lunar orbits

Detalhes bibliográficos
Autor(a) principal: Winter, O. C. [UNESP]
Data de Publicação: 2008
Outros Autores: Mourão, D. C., Melo, C. F., Giuliatti MacAu, E. N. [UNESP], Winter, S. M., Ferreira, J. L.
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://hdl.handle.net/11449/231914
Resumo: It is well known that lunar satellites in polar orbits suffer a high increase on the eccentricity due to the gravitational perturbation of the Earth. That effect is a natural consequence of the Lidov-Kozai resonance. The final fate of such satellites is the collision with the Moon. Therefore, the control of the orbital eccentricity leads to the control of the satellite's lifetime. In the present work we study this problem and introduce an approach in order to keep the orbital eccentricity of the satellite at low values. The whole work was made considering two systems: the 3-body problem, Moon-Earth-satellite and the 4-body problem, Moon-Earth-Sun-satellite. First, we simulated the systems considering a satellite with initial eccentricity equals to 0.0001 and a range of initial altitudes between 100km and 5000km. In such simulations we followed the evolution of the satellite's eccentricity. We also obtained an empirical expression for the length of time needed to occur the collision with the Moon as a function of the initial altitude. The results found for the 3-body model were not significantly different from those found for the 4-body model. Secondly, using low thrust propulsion, we introduced a correction of the eccentricity every time it reached the value 0.05. These simulations were made considering a set of different thrust values, from 0.1N up to 0.4N which can be obtained by using Hall Plasma Thrusters. In each run we measured the length of time, needed to correct the eccentricity value (from e = 0.04 to e = 0.05). From these results we obtained empirical expressions of this time as a function of the initial altitude and as a function of the thrust value.
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spelling Controlling the eccentricity of polar lunar orbitsIt is well known that lunar satellites in polar orbits suffer a high increase on the eccentricity due to the gravitational perturbation of the Earth. That effect is a natural consequence of the Lidov-Kozai resonance. The final fate of such satellites is the collision with the Moon. Therefore, the control of the orbital eccentricity leads to the control of the satellite's lifetime. In the present work we study this problem and introduce an approach in order to keep the orbital eccentricity of the satellite at low values. The whole work was made considering two systems: the 3-body problem, Moon-Earth-satellite and the 4-body problem, Moon-Earth-Sun-satellite. First, we simulated the systems considering a satellite with initial eccentricity equals to 0.0001 and a range of initial altitudes between 100km and 5000km. In such simulations we followed the evolution of the satellite's eccentricity. We also obtained an empirical expression for the length of time needed to occur the collision with the Moon as a function of the initial altitude. The results found for the 3-body model were not significantly different from those found for the 4-body model. Secondly, using low thrust propulsion, we introduced a correction of the eccentricity every time it reached the value 0.05. These simulations were made considering a set of different thrust values, from 0.1N up to 0.4N which can be obtained by using Hall Plasma Thrusters. In each run we measured the length of time, needed to correct the eccentricity value (from e = 0.04 to e = 0.05). From these results we obtained empirical expressions of this time as a function of the initial altitude and as a function of the thrust value.Grupo de Dinâmica Orbital and Planetologia São Paulo State University UNESP, Av. Ariberto Pereira da Cunha, 333, Guaratinguetá - SPInstitute de Física Universidade de Brasília - UnB, Brasilia - DFInstituto Nacional de Pesquisas Espaciais - INPE, Av. dos Astronautas, 1752, São José dos Campos -SPGrupo de Dinâmica Orbital and Planetologia São Paulo State University UNESP, Av. Ariberto Pereira da Cunha, 333, Guaratinguetá - SPUniversidade Estadual Paulista (UNESP)Universidade de Brasília (UnB)Instituto Nacional de Pesquisas Espaciais - INPEWinter, O. C. [UNESP]Mourão, D. C.Melo, C. F.Giuliatti MacAu, E. N. [UNESP]Winter, S. M.Ferreira, J. L.2022-04-29T08:48:11Z2022-04-29T08:48:11Z2008-12-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject4700-4708International Astronautical Federation - 59th International Astronautical Congress 2008, IAC 2008, v. 7, p. 4700-4708.http://hdl.handle.net/11449/2319142-s2.0-77950461921Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengInternational Astronautical Federation - 59th International Astronautical Congress 2008, IAC 2008info:eu-repo/semantics/openAccess2022-04-29T08:48:11Zoai:repositorio.unesp.br:11449/231914Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-29T08:48:11Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Controlling the eccentricity of polar lunar orbits
title Controlling the eccentricity of polar lunar orbits
spellingShingle Controlling the eccentricity of polar lunar orbits
Winter, O. C. [UNESP]
title_short Controlling the eccentricity of polar lunar orbits
title_full Controlling the eccentricity of polar lunar orbits
title_fullStr Controlling the eccentricity of polar lunar orbits
title_full_unstemmed Controlling the eccentricity of polar lunar orbits
title_sort Controlling the eccentricity of polar lunar orbits
author Winter, O. C. [UNESP]
author_facet Winter, O. C. [UNESP]
Mourão, D. C.
Melo, C. F.
Giuliatti MacAu, E. N. [UNESP]
Winter, S. M.
Ferreira, J. L.
author_role author
author2 Mourão, D. C.
Melo, C. F.
Giuliatti MacAu, E. N. [UNESP]
Winter, S. M.
Ferreira, J. L.
author2_role author
author
author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
Universidade de Brasília (UnB)
Instituto Nacional de Pesquisas Espaciais - INPE
dc.contributor.author.fl_str_mv Winter, O. C. [UNESP]
Mourão, D. C.
Melo, C. F.
Giuliatti MacAu, E. N. [UNESP]
Winter, S. M.
Ferreira, J. L.
description It is well known that lunar satellites in polar orbits suffer a high increase on the eccentricity due to the gravitational perturbation of the Earth. That effect is a natural consequence of the Lidov-Kozai resonance. The final fate of such satellites is the collision with the Moon. Therefore, the control of the orbital eccentricity leads to the control of the satellite's lifetime. In the present work we study this problem and introduce an approach in order to keep the orbital eccentricity of the satellite at low values. The whole work was made considering two systems: the 3-body problem, Moon-Earth-satellite and the 4-body problem, Moon-Earth-Sun-satellite. First, we simulated the systems considering a satellite with initial eccentricity equals to 0.0001 and a range of initial altitudes between 100km and 5000km. In such simulations we followed the evolution of the satellite's eccentricity. We also obtained an empirical expression for the length of time needed to occur the collision with the Moon as a function of the initial altitude. The results found for the 3-body model were not significantly different from those found for the 4-body model. Secondly, using low thrust propulsion, we introduced a correction of the eccentricity every time it reached the value 0.05. These simulations were made considering a set of different thrust values, from 0.1N up to 0.4N which can be obtained by using Hall Plasma Thrusters. In each run we measured the length of time, needed to correct the eccentricity value (from e = 0.04 to e = 0.05). From these results we obtained empirical expressions of this time as a function of the initial altitude and as a function of the thrust value.
publishDate 2008
dc.date.none.fl_str_mv 2008-12-01
2022-04-29T08:48:11Z
2022-04-29T08:48:11Z
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 International Astronautical Federation - 59th International Astronautical Congress 2008, IAC 2008, v. 7, p. 4700-4708.
http://hdl.handle.net/11449/231914
2-s2.0-77950461921
identifier_str_mv International Astronautical Federation - 59th International Astronautical Congress 2008, IAC 2008, v. 7, p. 4700-4708.
2-s2.0-77950461921
url http://hdl.handle.net/11449/231914
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv International Astronautical Federation - 59th International Astronautical Congress 2008, IAC 2008
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 4700-4708
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
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reponame_str 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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