Tidal evolution of close-in exoplanets in co-orbital configurations
- Autores
- Rodríguez, Adrian; Giuppone, Cristian Andrés; Michtchenko, Tatiana A.
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In this paper, we study the behavior of a pair of co-orbital planets, both orbiting a central star on the same plane and undergoing tidal interactions. Our goal is to investigate final orbital configurations of the planets, initially involved in the 1/1 mean-motion resonance (MMR), after long-lasting tidal evolution. The study is done in the form of purely numerical simulations of the exact equations of motions accounting for gravitational and tidal forces. The results obtained show that, at least for equal mass planets, the combined effects of the resonant and tidal interactions provoke the orbital instability of the system, often resulting in collision between the planets. We first discuss the case of two hot-super-Earth planets, whose orbital dynamics can be easily understood in the frame of our semi-analytical model of the 1/1 MMR. Systems consisting of two hot-Saturn planets are also briefly discussed.
Fil: Rodríguez, Adrian. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; Brasil
Fil: Giuppone, Cristian Andrés. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Michtchenko, Tatiana A.. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; Brasil - Materia
-
Celestial Mechanics
Planets And Satellites
Tides
Exo-Trojans - 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:11336/25845
Ver los metadatos del registro completo
id |
CONICETDig_44564b4bd0b8eb151cfe1061825f9d13 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/25845 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
Tidal evolution of close-in exoplanets in co-orbital configurationsRodríguez, AdrianGiuppone, Cristian AndrésMichtchenko, Tatiana A.Celestial MechanicsPlanets And SatellitesTidesExo-Trojanshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this paper, we study the behavior of a pair of co-orbital planets, both orbiting a central star on the same plane and undergoing tidal interactions. Our goal is to investigate final orbital configurations of the planets, initially involved in the 1/1 mean-motion resonance (MMR), after long-lasting tidal evolution. The study is done in the form of purely numerical simulations of the exact equations of motions accounting for gravitational and tidal forces. The results obtained show that, at least for equal mass planets, the combined effects of the resonant and tidal interactions provoke the orbital instability of the system, often resulting in collision between the planets. We first discuss the case of two hot-super-Earth planets, whose orbital dynamics can be easily understood in the frame of our semi-analytical model of the 1/1 MMR. Systems consisting of two hot-Saturn planets are also briefly discussed.Fil: Rodríguez, Adrian. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; BrasilFil: Giuppone, Cristian Andrés. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Michtchenko, Tatiana A.. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; BrasilSpringer2013-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/25845Rodríguez, Adrian; Giuppone, Cristian Andrés; Michtchenko, Tatiana A.; Tidal evolution of close-in exoplanets in co-orbital configurations; Springer; Celestial Mechanics & Dynamical Astronomy; 117; 1; 7-2013; 59-740923-2958CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10569-013-9502-yinfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10569-013-9502-yinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1306.4293info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:13:07Zoai:ri.conicet.gov.ar:11336/25845instacron: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 10:13:07.897CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Tidal evolution of close-in exoplanets in co-orbital configurations |
title |
Tidal evolution of close-in exoplanets in co-orbital configurations |
spellingShingle |
Tidal evolution of close-in exoplanets in co-orbital configurations Rodríguez, Adrian Celestial Mechanics Planets And Satellites Tides Exo-Trojans |
title_short |
Tidal evolution of close-in exoplanets in co-orbital configurations |
title_full |
Tidal evolution of close-in exoplanets in co-orbital configurations |
title_fullStr |
Tidal evolution of close-in exoplanets in co-orbital configurations |
title_full_unstemmed |
Tidal evolution of close-in exoplanets in co-orbital configurations |
title_sort |
Tidal evolution of close-in exoplanets in co-orbital configurations |
dc.creator.none.fl_str_mv |
Rodríguez, Adrian Giuppone, Cristian Andrés Michtchenko, Tatiana A. |
author |
Rodríguez, Adrian |
author_facet |
Rodríguez, Adrian Giuppone, Cristian Andrés Michtchenko, Tatiana A. |
author_role |
author |
author2 |
Giuppone, Cristian Andrés Michtchenko, Tatiana A. |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Celestial Mechanics Planets And Satellites Tides Exo-Trojans |
topic |
Celestial Mechanics Planets And Satellites Tides Exo-Trojans |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
In this paper, we study the behavior of a pair of co-orbital planets, both orbiting a central star on the same plane and undergoing tidal interactions. Our goal is to investigate final orbital configurations of the planets, initially involved in the 1/1 mean-motion resonance (MMR), after long-lasting tidal evolution. The study is done in the form of purely numerical simulations of the exact equations of motions accounting for gravitational and tidal forces. The results obtained show that, at least for equal mass planets, the combined effects of the resonant and tidal interactions provoke the orbital instability of the system, often resulting in collision between the planets. We first discuss the case of two hot-super-Earth planets, whose orbital dynamics can be easily understood in the frame of our semi-analytical model of the 1/1 MMR. Systems consisting of two hot-Saturn planets are also briefly discussed. Fil: Rodríguez, Adrian. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; Brasil Fil: Giuppone, Cristian Andrés. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Michtchenko, Tatiana A.. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; Brasil |
description |
In this paper, we study the behavior of a pair of co-orbital planets, both orbiting a central star on the same plane and undergoing tidal interactions. Our goal is to investigate final orbital configurations of the planets, initially involved in the 1/1 mean-motion resonance (MMR), after long-lasting tidal evolution. The study is done in the form of purely numerical simulations of the exact equations of motions accounting for gravitational and tidal forces. The results obtained show that, at least for equal mass planets, the combined effects of the resonant and tidal interactions provoke the orbital instability of the system, often resulting in collision between the planets. We first discuss the case of two hot-super-Earth planets, whose orbital dynamics can be easily understood in the frame of our semi-analytical model of the 1/1 MMR. Systems consisting of two hot-Saturn planets are also briefly discussed. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-07 |
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/11336/25845 Rodríguez, Adrian; Giuppone, Cristian Andrés; Michtchenko, Tatiana A.; Tidal evolution of close-in exoplanets in co-orbital configurations; Springer; Celestial Mechanics & Dynamical Astronomy; 117; 1; 7-2013; 59-74 0923-2958 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/25845 |
identifier_str_mv |
Rodríguez, Adrian; Giuppone, Cristian Andrés; Michtchenko, Tatiana A.; Tidal evolution of close-in exoplanets in co-orbital configurations; Springer; Celestial Mechanics & Dynamical Astronomy; 117; 1; 7-2013; 59-74 0923-2958 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1007/s10569-013-9502-y info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10569-013-9502-y info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1306.4293 |
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 application/pdf |
dc.publisher.none.fl_str_mv |
Springer |
publisher.none.fl_str_mv |
Springer |
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 |
_version_ |
1844614044684648448 |
score |
13.070432 |