A study of distant retrograde orbits in the neighborhood of the moon

Detalhes bibliográficos
Autor(a) principal: Winter, Othon C. [UNESP]
Data de Publicação: 2020
Outros Autores: Pires, Pryscilla
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://hdl.handle.net/11449/233095
Resumo: In this work, we have numerically investigated a region of retrograde orbits around the Moon in the light of the four-body Sun-Earth-Moon-particle problem. In this context, the gravitation effects of the Sun was taken into account, and the Earth and the Moon assumed their realistic orbital parameters. From this study we identified initial conditions for lunar Distant Retrograde Orbits (DROs) that remain bounded after propagating a conservative quantity of 20 years. By comparing our results with the results obtained in the Circular Restricted Three Body Problem (CRTBP) we see a substantial loss of particles, the region of stability diminished to 4% the original size encountered for the CRTBP. This set of lunar DROs has initial velocities around 0.5 (y-axis) and initial values of x around 0.8 in the rotating Earth-Moon frame. Regarding their initial lunar orbital elements, their eccentricities follows the equation e = 2.25963x10-6 a + 0.23845 (standard error of 1%), while their initial semi-major axis values are between 110,000 and 185,000 Km.
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spelling A study of distant retrograde orbits in the neighborhood of the moonEarthMoonOrbitsIn this work, we have numerically investigated a region of retrograde orbits around the Moon in the light of the four-body Sun-Earth-Moon-particle problem. In this context, the gravitation effects of the Sun was taken into account, and the Earth and the Moon assumed their realistic orbital parameters. From this study we identified initial conditions for lunar Distant Retrograde Orbits (DROs) that remain bounded after propagating a conservative quantity of 20 years. By comparing our results with the results obtained in the Circular Restricted Three Body Problem (CRTBP) we see a substantial loss of particles, the region of stability diminished to 4% the original size encountered for the CRTBP. This set of lunar DROs has initial velocities around 0.5 (y-axis) and initial values of x around 0.8 in the rotating Earth-Moon frame. Regarding their initial lunar orbital elements, their eccentricities follows the equation e = 2.25963x10-6 a + 0.23845 (standard error of 1%), while their initial semi-major axis values are between 110,000 and 185,000 Km.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Department of Mathematics São Paulo State University, 333 Av. Ariberto Pereira da CunhaDepartment of Mathematics Physics and Computing Rio de Janeiro State University, Rod. Pres. Dutra, km 298 - Polo IndustrialDepartment of Mathematics São Paulo State University, 333 Av. Ariberto Pereira da CunhaCNPq: 305210/2018-1Universidade Estadual Paulista (UNESP)Rio de Janeiro State UniversityWinter, Othon C. [UNESP]Pires, Pryscilla2022-05-01T03:42:45Z2022-05-01T03:42:45Z2020-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectProceedings of the International Astronautical Congress, IAC, v. 2020-October.0074-1795http://hdl.handle.net/11449/2330952-s2.0-85100921469Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengProceedings of the International Astronautical Congress, IACinfo:eu-repo/semantics/openAccess2024-07-02T14:29:48Zoai:repositorio.unesp.br:11449/233095Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T20:06:46.445527Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv A study of distant retrograde orbits in the neighborhood of the moon
title A study of distant retrograde orbits in the neighborhood of the moon
spellingShingle A study of distant retrograde orbits in the neighborhood of the moon
Winter, Othon C. [UNESP]
Earth
Moon
Orbits
title_short A study of distant retrograde orbits in the neighborhood of the moon
title_full A study of distant retrograde orbits in the neighborhood of the moon
title_fullStr A study of distant retrograde orbits in the neighborhood of the moon
title_full_unstemmed A study of distant retrograde orbits in the neighborhood of the moon
title_sort A study of distant retrograde orbits in the neighborhood of the moon
author Winter, Othon C. [UNESP]
author_facet Winter, Othon C. [UNESP]
Pires, Pryscilla
author_role author
author2 Pires, Pryscilla
author2_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
Rio de Janeiro State University
dc.contributor.author.fl_str_mv Winter, Othon C. [UNESP]
Pires, Pryscilla
dc.subject.por.fl_str_mv Earth
Moon
Orbits
topic Earth
Moon
Orbits
description In this work, we have numerically investigated a region of retrograde orbits around the Moon in the light of the four-body Sun-Earth-Moon-particle problem. In this context, the gravitation effects of the Sun was taken into account, and the Earth and the Moon assumed their realistic orbital parameters. From this study we identified initial conditions for lunar Distant Retrograde Orbits (DROs) that remain bounded after propagating a conservative quantity of 20 years. By comparing our results with the results obtained in the Circular Restricted Three Body Problem (CRTBP) we see a substantial loss of particles, the region of stability diminished to 4% the original size encountered for the CRTBP. This set of lunar DROs has initial velocities around 0.5 (y-axis) and initial values of x around 0.8 in the rotating Earth-Moon frame. Regarding their initial lunar orbital elements, their eccentricities follows the equation e = 2.25963x10-6 a + 0.23845 (standard error of 1%), while their initial semi-major axis values are between 110,000 and 185,000 Km.
publishDate 2020
dc.date.none.fl_str_mv 2020-01-01
2022-05-01T03:42:45Z
2022-05-01T03:42:45Z
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 Proceedings of the International Astronautical Congress, IAC, v. 2020-October.
0074-1795
http://hdl.handle.net/11449/233095
2-s2.0-85100921469
identifier_str_mv Proceedings of the International Astronautical Congress, IAC, v. 2020-October.
0074-1795
2-s2.0-85100921469
url http://hdl.handle.net/11449/233095
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Proceedings of the International Astronautical Congress, IAC
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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