A numerical study of the 1/2, 2/1, and 1/1 retrograde mean motion resonances in planetary systems

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dc.contributor.authorCarita, Gabriel Antonio [UNESP]
dc.contributor.authorSignor, Alan Cefali [UNESP]
dc.contributor.authorMorais, Maria Helena Moreira [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2022-11-30T13:40:42Z
dc.date.available2022-11-30T13:40:42Z
dc.date.issued2022-07-29
dc.description.abstractWe present a numerical study on the stability of the 1/2, 2/1, and 1/1 retrograde mean motion resonances in the three-body problem composed of a solar mass star, a Jupiter mass planet, and an additional body with zero mass (elliptic restricted three-body problem) or masses corresponding to either Neptune, Saturn, or Jupiter (planetary three-body problem). For each system, we obtain stability maps using the n-body numerical integrator REBOUND and computing the chaos indicator mean exponential growth factor of nearby orbits (MEGNO). We show that families of periodic orbits exist in all configurations and they correspond to the libration of either a single resonant argument or all resonant arguments (fixed points). We compare the results obtained in the elliptic restricted three-body problem with previous results in the literature, and we show the differences and similarities between the phase space topology for these retrograde resonances in the circular restricted, elliptic restricted, and planetary three-body problems.en
dc.description.affiliationUniv Estadual Paulista UNESP, Inst Geociencias & Ciencias Exatas, Av 24-A,1515, BR-13506900 Rio Claro, SP, Brazil
dc.description.affiliationUnespUniv Estadual Paulista UNESP, Inst Geociencias & Ciencias Exatas, Av 24-A,1515, BR-13506900 Rio Claro, SP, Brazil
dc.description.sponsorshipCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipIdCAPES: 001
dc.description.sponsorshipIdCNPq: PQ2/304037/2018-4
dc.description.sponsorshipIdFAPESP: FAPESP/2019/24958-5
dc.description.sponsorshipIdFAPESP: FAPESP/2021/11982-5
dc.format.extent2280-2292
dc.identifierhttp://dx.doi.org/10.1093/mnras/stac1606
dc.identifier.citationMonthly Notices Of The Royal Astronomical Society. Oxford: Oxford Univ Press, v. 515, n. 2, p. 2280-2292, 2022.
dc.identifier.doi10.1093/mnras/stac1606
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/11449/237643
dc.identifier.wosWOS:000834368400001
dc.language.isoeng
dc.publisherOxford Univ Press
dc.relation.ispartofMonthly Notices Of The Royal Astronomical Society
dc.sourceWeb of Science
dc.subjectChaos
dc.subjectmethods: numerical
dc.subjectPlanets and satellites: dynamical evolution and stability
dc.subject(stars:) planetary systems
dc.titleA numerical study of the 1/2, 2/1, and 1/1 retrograde mean motion resonances in planetary systemsen
dc.typeArtigo
dcterms.licensehttp://www.oxfordjournals.org/access_purchase/self-archiving_policyb.html
dcterms.rightsHolderOxford Univ Press
unesp.author.orcid0000-0001-5333-2736[3]

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