A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits

Autores
Giuppone, Cristian Andrés; Morais, M.H.M.; Correia, A.C.M.
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We test a crossing orbit stability criterion for eccentric planetary systems, based on Wisdom´s criterion of first order mean motion resonance overlap citep{Wisdom1980AJ}. We show that this criterion fits the stability regions in real exoplanet systems quite well. In addition, we show that elliptical orbits can remain stable even for regions where the apocenter distance of the inner orbit is larger than the pericenter distance of the outer orbit, as long as the initial orbits are aligned. The analytical expressions provided here can be used to put rapid constraints on the stability zones of multi-planetary systems. As a byproduct of this research, we further show that the amplitude variations of the eccentricity can be used as a fast-computing stability indicator.
Fil: Giuppone, Cristian Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina; Universidade de Aveiro. Departamento de Física, I3N; Portugal;
Fil: Morais, M.H.M.. Universidade de Aveiro. Departamento de Física, I3N; Portugal;
Fil: Correia, A.C.M.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia; Universidade de Aveiro. Departamento de Física, I3N; Portugal;
Materia
celestial mechanics
methods: numerical and analytical
stability
exoplanets
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/2470

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network_name_str CONICET Digital (CONICET)
spelling A semi-empirical stability criterion for real multi-planetary systems with eccentric orbitsGiuppone, Cristian AndrésMorais, M.H.M.Correia, A.C.M.celestial mechanicsmethods: numerical and analyticalstabilityexoplanetshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We test a crossing orbit stability criterion for eccentric planetary systems, based on Wisdom´s criterion of first order mean motion resonance overlap citep{Wisdom1980AJ}. We show that this criterion fits the stability regions in real exoplanet systems quite well. In addition, we show that elliptical orbits can remain stable even for regions where the apocenter distance of the inner orbit is larger than the pericenter distance of the outer orbit, as long as the initial orbits are aligned. The analytical expressions provided here can be used to put rapid constraints on the stability zones of multi-planetary systems. As a byproduct of this research, we further show that the amplitude variations of the eccentricity can be used as a fast-computing stability indicator.Fil: Giuppone, Cristian Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina; Universidade de Aveiro. Departamento de Física, I3N; Portugal;Fil: Morais, M.H.M.. Universidade de Aveiro. Departamento de Física, I3N; Portugal;Fil: Correia, A.C.M.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia; Universidade de Aveiro. Departamento de Física, I3N; Portugal;Wiley-blackwell Publishing, Inc2013-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/2470Giuppone, Cristian Andrés; Morais, M.H.M.; Correia, A.C.M.; A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits; Wiley-blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 12-2013; 3547-35560035-8711enginfo:eu-repo/semantics/reference es info:eu-repo/semantics/reference/arxiv/1309.6861v1 [astro-ph.EP]info:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1309.6861info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:41:15Zoai:ri.conicet.gov.ar:11336/2470instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:41:15.722CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
title A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
spellingShingle A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
Giuppone, Cristian Andrés
celestial mechanics
methods: numerical and analytical
stability
exoplanets
title_short A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
title_full A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
title_fullStr A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
title_full_unstemmed A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
title_sort A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits
dc.creator.none.fl_str_mv Giuppone, Cristian Andrés
Morais, M.H.M.
Correia, A.C.M.
author Giuppone, Cristian Andrés
author_facet Giuppone, Cristian Andrés
Morais, M.H.M.
Correia, A.C.M.
author_role author
author2 Morais, M.H.M.
Correia, A.C.M.
author2_role author
author
dc.subject.none.fl_str_mv celestial mechanics
methods: numerical and analytical
stability
exoplanets
topic celestial mechanics
methods: numerical and analytical
stability
exoplanets
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We test a crossing orbit stability criterion for eccentric planetary systems, based on Wisdom´s criterion of first order mean motion resonance overlap citep{Wisdom1980AJ}. We show that this criterion fits the stability regions in real exoplanet systems quite well. In addition, we show that elliptical orbits can remain stable even for regions where the apocenter distance of the inner orbit is larger than the pericenter distance of the outer orbit, as long as the initial orbits are aligned. The analytical expressions provided here can be used to put rapid constraints on the stability zones of multi-planetary systems. As a byproduct of this research, we further show that the amplitude variations of the eccentricity can be used as a fast-computing stability indicator.
Fil: Giuppone, Cristian Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina; Universidade de Aveiro. Departamento de Física, I3N; Portugal;
Fil: Morais, M.H.M.. Universidade de Aveiro. Departamento de Física, I3N; Portugal;
Fil: Correia, A.C.M.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia; Universidade de Aveiro. Departamento de Física, I3N; Portugal;
description We test a crossing orbit stability criterion for eccentric planetary systems, based on Wisdom´s criterion of first order mean motion resonance overlap citep{Wisdom1980AJ}. We show that this criterion fits the stability regions in real exoplanet systems quite well. In addition, we show that elliptical orbits can remain stable even for regions where the apocenter distance of the inner orbit is larger than the pericenter distance of the outer orbit, as long as the initial orbits are aligned. The analytical expressions provided here can be used to put rapid constraints on the stability zones of multi-planetary systems. As a byproduct of this research, we further show that the amplitude variations of the eccentricity can be used as a fast-computing stability indicator.
publishDate 2013
dc.date.none.fl_str_mv 2013-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/2470
Giuppone, Cristian Andrés; Morais, M.H.M.; Correia, A.C.M.; A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits; Wiley-blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 12-2013; 3547-3556
0035-8711
url http://hdl.handle.net/11336/2470
identifier_str_mv Giuppone, Cristian Andrés; Morais, M.H.M.; Correia, A.C.M.; A semi-empirical stability criterion for real multi-planetary systems with eccentric orbits; Wiley-blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 12-2013; 3547-3556
0035-8711
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/reference es info:eu-repo/semantics/reference/arxiv/1309.6861v1 [astro-ph.EP]
info:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1309.6861
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Wiley-blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley-blackwell Publishing, Inc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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