A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems

Detalhes bibliográficos
Autor(a) principal: Signor, Alan Cefali [UNESP]
Data de Publicação: 2023
Outros Autores: Caritá, Gabriel Antonio [UNESP], Morais, Maria Helena Moreira [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1093/mnras/stad336
http://hdl.handle.net/11449/247363
Resumo: We present a numerical study on the stability of all fourth- and fifth-order retrograde mean motion resonances (1/3, 3/1, 1/4, 4/1, 2/3, and 3/2) in the 3-body problem composed of a solar mass star, a Jupiter mass planet, and an additional body with zero mass (elliptic restricted problem) or masses corresponding to either Neptune, Saturn, or Jupiter (planetary problem). The fixed point families exist in all cases and are identified through libration of all resonant angles simultaneously. In addition, configurations with libration of a single resonant angle were also observed. Our results for the elliptic restricted 3-body problem are in agreement with previous studies of retrograde periodic orbits, but we also observe new families not previously reported. Our results regarding stable resonant retrograde configurations in the planetary 3-body problem could be applicable to extra-Solar systems.
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spelling A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systemsmethods: numericalplanetary systemsplanets and satellites: dynamical evolution and stabilityWe present a numerical study on the stability of all fourth- and fifth-order retrograde mean motion resonances (1/3, 3/1, 1/4, 4/1, 2/3, and 3/2) in the 3-body problem composed of a solar mass star, a Jupiter mass planet, and an additional body with zero mass (elliptic restricted problem) or masses corresponding to either Neptune, Saturn, or Jupiter (planetary problem). The fixed point families exist in all cases and are identified through libration of all resonant angles simultaneously. In addition, configurations with libration of a single resonant angle were also observed. Our results for the elliptic restricted 3-body problem are in agreement with previous studies of retrograde periodic orbits, but we also observe new families not previously reported. Our results regarding stable resonant retrograde configurations in the planetary 3-body problem could be applicable to extra-Solar systems.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Instituto de Geociências e Ciências Exatas Universidade Estadual Paulista (UNESP), Avenida 24-A, 1515, SPDivisão de Mecânica Espacial e Controle INPE, SPInstituto de Geociências e Ciências Exatas Universidade Estadual Paulista (UNESP), Avenida 24-A, 1515, SPCAPES: 88887.675709/2022-00FAPESP: FAPESP/2021/11982-5FAPESP: FAPESP/2022/08716-4Universidade Estadual Paulista (UNESP)INPESignor, Alan Cefali [UNESP]Caritá, Gabriel Antonio [UNESP]Morais, Maria Helena Moreira [UNESP]2023-07-29T13:14:00Z2023-07-29T13:14:00Z2023-04-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article4696-4714http://dx.doi.org/10.1093/mnras/stad336Monthly Notices of the Royal Astronomical Society, v. 520, n. 3, p. 4696-4714, 2023.1365-29660035-8711http://hdl.handle.net/11449/24736310.1093/mnras/stad3362-s2.0-85159189939Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengMonthly Notices of the Royal Astronomical Societyinfo:eu-repo/semantics/openAccess2023-07-29T13:14:00Zoai:repositorio.unesp.br:11449/247363Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T19:48:53.475268Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
title A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
spellingShingle A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
Signor, Alan Cefali [UNESP]
methods: numerical
planetary systems
planets and satellites: dynamical evolution and stability
title_short A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
title_full A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
title_fullStr A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
title_full_unstemmed A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
title_sort A numerical study of fourth- And fifth-order retrograde mean motion resonances in planetary systems
author Signor, Alan Cefali [UNESP]
author_facet Signor, Alan Cefali [UNESP]
Caritá, Gabriel Antonio [UNESP]
Morais, Maria Helena Moreira [UNESP]
author_role author
author2 Caritá, Gabriel Antonio [UNESP]
Morais, Maria Helena Moreira [UNESP]
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
INPE
dc.contributor.author.fl_str_mv Signor, Alan Cefali [UNESP]
Caritá, Gabriel Antonio [UNESP]
Morais, Maria Helena Moreira [UNESP]
dc.subject.por.fl_str_mv methods: numerical
planetary systems
planets and satellites: dynamical evolution and stability
topic methods: numerical
planetary systems
planets and satellites: dynamical evolution and stability
description We present a numerical study on the stability of all fourth- and fifth-order retrograde mean motion resonances (1/3, 3/1, 1/4, 4/1, 2/3, and 3/2) in the 3-body problem composed of a solar mass star, a Jupiter mass planet, and an additional body with zero mass (elliptic restricted problem) or masses corresponding to either Neptune, Saturn, or Jupiter (planetary problem). The fixed point families exist in all cases and are identified through libration of all resonant angles simultaneously. In addition, configurations with libration of a single resonant angle were also observed. Our results for the elliptic restricted 3-body problem are in agreement with previous studies of retrograde periodic orbits, but we also observe new families not previously reported. Our results regarding stable resonant retrograde configurations in the planetary 3-body problem could be applicable to extra-Solar systems.
publishDate 2023
dc.date.none.fl_str_mv 2023-07-29T13:14:00Z
2023-07-29T13:14:00Z
2023-04-01
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/10.1093/mnras/stad336
Monthly Notices of the Royal Astronomical Society, v. 520, n. 3, p. 4696-4714, 2023.
1365-2966
0035-8711
http://hdl.handle.net/11449/247363
10.1093/mnras/stad336
2-s2.0-85159189939
url http://dx.doi.org/10.1093/mnras/stad336
http://hdl.handle.net/11449/247363
identifier_str_mv Monthly Notices of the Royal Astronomical Society, v. 520, n. 3, p. 4696-4714, 2023.
1365-2966
0035-8711
10.1093/mnras/stad336
2-s2.0-85159189939
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 4696-4714
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
_version_ 1808129121749827584

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