Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion

Detalhes bibliográficos
Autor(a) principal: Winter, O. C. [UNESP]
Data de Publicação: 2009
Outros Autores: Mourao, D. C. [UNESP], Melo, C. F. [UNESP], Macau, E. N., Ferreira, J. L., Carvalho, J. P. S. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1155/2009/159287
http://hdl.handle.net/11449/42366
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 100 km and 5000 km. 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. Copyright (C) 2009 O. C. Winter et al.
id UNSP_3972696b51d0dc9dfa890369affd71de
oai_identifier_str oai:repositorio.unesp.br:11449/42366
network_acronym_str UNSP
network_name_str Repositório Institucional da UNESP
repository_id_str 2946
spelling Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust PropulsionIt 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 100 km and 5000 km. 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. Copyright (C) 2009 O. C. Winter et al.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Agência Espacial Brasileira (AEB)Univ Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, BrazilINPE, Sao Jose Dos Campos, SP, BrazilUniv Brasilia UnB, Inst Fis, BR-70919970 Brasilia, DF, BrazilUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, BrazilHindawi Publishing CorporationUniversidade Estadual Paulista (Unesp)Instituto Nacional de Pesquisas Espaciais (INPE)Universidade de Brasília (UnB)Winter, O. C. [UNESP]Mourao, D. C. [UNESP]Melo, C. F. [UNESP]Macau, E. N.Ferreira, J. L.Carvalho, J. P. S. [UNESP]2014-05-20T15:33:56Z2014-05-20T15:33:56Z2009-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article10application/pdfhttp://dx.doi.org/10.1155/2009/159287Mathematical Problems In Engineering. New York: Hindawi Publishing Corporation, p. 10, 2009.1024-123Xhttp://hdl.handle.net/11449/4236610.1155/2009/159287WOS:000277590300001WOS000277590300001.pdf0960024575647258Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengMathematical Problems in Engineering1.145info:eu-repo/semantics/openAccess2023-12-03T06:12:06Zoai:repositorio.unesp.br:11449/42366Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-12-03T06:12:06Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
title Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
spellingShingle Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
Winter, O. C. [UNESP]
title_short Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
title_full Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
title_fullStr Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
title_full_unstemmed Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
title_sort Controlling the Eccentricity of Polar Lunar Orbits with Low-Thrust Propulsion
author Winter, O. C. [UNESP]
author_facet Winter, O. C. [UNESP]
Mourao, D. C. [UNESP]
Melo, C. F. [UNESP]
Macau, E. N.
Ferreira, J. L.
Carvalho, J. P. S. [UNESP]
author_role author
author2 Mourao, D. C. [UNESP]
Melo, C. F. [UNESP]
Macau, E. N.
Ferreira, J. L.
Carvalho, J. P. S. [UNESP]
author2_role author
author
author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Instituto Nacional de Pesquisas Espaciais (INPE)
Universidade de Brasília (UnB)
dc.contributor.author.fl_str_mv Winter, O. C. [UNESP]
Mourao, D. C. [UNESP]
Melo, C. F. [UNESP]
Macau, E. N.
Ferreira, J. L.
Carvalho, J. P. S. [UNESP]
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 100 km and 5000 km. 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. Copyright (C) 2009 O. C. Winter et al.
publishDate 2009
dc.date.none.fl_str_mv 2009-01-01
2014-05-20T15:33:56Z
2014-05-20T15:33:56Z
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/10.1155/2009/159287
Mathematical Problems In Engineering. New York: Hindawi Publishing Corporation, p. 10, 2009.
1024-123X
http://hdl.handle.net/11449/42366
10.1155/2009/159287
WOS:000277590300001
WOS000277590300001.pdf
0960024575647258
url http://dx.doi.org/10.1155/2009/159287
http://hdl.handle.net/11449/42366
identifier_str_mv Mathematical Problems In Engineering. New York: Hindawi Publishing Corporation, p. 10, 2009.
1024-123X
10.1155/2009/159287
WOS:000277590300001
WOS000277590300001.pdf
0960024575647258
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Mathematical Problems in Engineering
1.145
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 10
application/pdf
dc.publisher.none.fl_str_mv Hindawi Publishing Corporation
publisher.none.fl_str_mv Hindawi Publishing Corporation
dc.source.none.fl_str_mv Web of Science
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
_version_ 1799965153576353792