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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/2470
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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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1844614442886627328 |
score |
13.070432 |