A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering
- Autores
- Bonomo, A. S.; Hébrard, G.; Raymond, S. N.; Bouchy, F.; Lecavelier Des Etangs, A.; Bordé, P.; Aigrain, S.; Almenara, J. M.; Alonso, R.; Cabrera, J.; Csizmadia, Sz.; Damiani, C.; Deeg, H. J.; Deleuil, M.; Diaz, Rodrigo Fernando; Erikson, A.; Fridlund, M.; Gandolfi, D.; Guenther, E.; Guillot, T.; Hatzes, A.; Izidoro, A.; Lovis, C.; Moutou, C.; Ollivier, M.; Pätzold, M.; Rauer, H.; Rouan, D.; Santerne, A.; Schneider, J.
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- CoRoT-9b is one of the rare long-period (P = 95.3 days) transiting giant planets with a measured mass known to date. We present a new analysis of the CoRoT-9 system based on five years of radial-velocity (RV) monitoring with HARPS and three new space-based transits observed with CoRoT and Spitzer. Combining our new data with already published measurements we redetermine the CoRoT-9 system parameters and find good agreement with the published values. We uncover a higher significance for the small but non-zero eccentricity of CoRoT-9b () and find no evidence for additional planets in the system. We use simulations of planet-planet scattering to show that the eccentricity of CoRoT-9b may have been generated by an instability in which a ∼ 50 M⊕ planet was ejected from the system. This scattering would not have produced a spin-orbit misalignment, so we predict that the CoRoT-9b orbit should lie within a few degrees of the initial plane of the protoplanetary disk. As a consequence, any significant stellar obliquity would indicate that the disk was primordially tilted.
Fil: Bonomo, A. S.. Istituto Nazionale Di Astrofisica; Italia
Fil: Hébrard, G.. Universite de Paris I Pantheon - Sorbonne; Francia
Fil: Raymond, S. N.. Laboratoire D; Francia
Fil: Bouchy, F.. Universidad de Ginebra; Suiza
Fil: Lecavelier Des Etangs, A.. Universite de Paris I Pantheon - Sorbonne; Francia
Fil: Bordé, P.. Laboratoire D; Francia
Fil: Aigrain, S.. University of Oxford; Reino Unido
Fil: Almenara, J. M.. Universidad de Ginebra; Suiza
Fil: Alonso, R.. Universidad de la Laguna; España
Fil: Cabrera, J.. Deutsches Zentrum Fur Luft- Und Raumfahrt; Alemania
Fil: Csizmadia, Sz.. Deutsches Zentrum Fur Luft- Und Raumfahrt; Alemania
Fil: Damiani, C.. Université de Paris XI; Francia
Fil: Deeg, H. J.. Universidad de la Laguna; España
Fil: Deleuil, M.. Laboratoire D; Francia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Erikson, A.. Deutsches Zentrum Fur Luft- Und Raumfahrt; Alemania
Fil: Fridlund, M.. Leiden Observatory Research Institute; Países Bajos
Fil: Gandolfi, D.. Università di Torino; Italia
Fil: Guenther, E.. Thüringer Landessternwarte; Alemania
Fil: Guillot, T.. Observatoire de la Cote D; Francia
Fil: Hatzes, A.. Thüringer Landessternwarte; Alemania
Fil: Izidoro, A.. Unesp-universidade Estadual Paulista; Brasil
Fil: Lovis, C.. Universidad de Ginebra; Suiza
Fil: Moutou, C.. Laboratoire D; Francia
Fil: Ollivier, M.. Université de Paris XI; Francia
Fil: Pätzold, M.. Universitat Zu Köln; Alemania
Fil: Rauer, H.. Technishe Universitat Berlin; Alemania
Fil: Rouan, D.. Lesia - Laboratoire D; Francia
Fil: Santerne, A.. Aix Marseille Université; Francia
Fil: Schneider, J.. Université Paris Diderot - Paris 7; Francia - Materia
-
PLANETARY SYSTEMS
STARS: INDIVIDUAL: COROT-9
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES - 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:11336/23612
Ver los metadatos del registro completo
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A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scatteringBonomo, A. S.Hébrard, G.Raymond, S. N.Bouchy, F.Lecavelier Des Etangs, A.Bordé, P.Aigrain, S.Almenara, J. M.Alonso, R.Cabrera, J.Csizmadia, Sz.Damiani, C.Deeg, H. J.Deleuil, M.Diaz, Rodrigo FernandoErikson, A.Fridlund, M.Gandolfi, D.Guenther, E.Guillot, T.Hatzes, A.Izidoro, A.Lovis, C.Moutou, C.Ollivier, M.Pätzold, M.Rauer, H.Rouan, D.Santerne, A.Schneider, J.PLANETARY SYSTEMSSTARS: INDIVIDUAL: COROT-9TECHNIQUES: PHOTOMETRICTECHNIQUES: RADIAL VELOCITIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1CoRoT-9b is one of the rare long-period (P = 95.3 days) transiting giant planets with a measured mass known to date. We present a new analysis of the CoRoT-9 system based on five years of radial-velocity (RV) monitoring with HARPS and three new space-based transits observed with CoRoT and Spitzer. Combining our new data with already published measurements we redetermine the CoRoT-9 system parameters and find good agreement with the published values. We uncover a higher significance for the small but non-zero eccentricity of CoRoT-9b () and find no evidence for additional planets in the system. We use simulations of planet-planet scattering to show that the eccentricity of CoRoT-9b may have been generated by an instability in which a ∼ 50 M⊕ planet was ejected from the system. This scattering would not have produced a spin-orbit misalignment, so we predict that the CoRoT-9b orbit should lie within a few degrees of the initial plane of the protoplanetary disk. As a consequence, any significant stellar obliquity would indicate that the disk was primordially tilted.Fil: Bonomo, A. S.. Istituto Nazionale Di Astrofisica; ItaliaFil: Hébrard, G.. Universite de Paris I Pantheon - Sorbonne; FranciaFil: Raymond, S. N.. Laboratoire D; FranciaFil: Bouchy, F.. Universidad de Ginebra; SuizaFil: Lecavelier Des Etangs, A.. Universite de Paris I Pantheon - Sorbonne; FranciaFil: Bordé, P.. Laboratoire D; FranciaFil: Aigrain, S.. University of Oxford; Reino UnidoFil: Almenara, J. M.. Universidad de Ginebra; SuizaFil: Alonso, R.. Universidad de la Laguna; EspañaFil: Cabrera, J.. Deutsches Zentrum Fur Luft- Und Raumfahrt; AlemaniaFil: Csizmadia, Sz.. Deutsches Zentrum Fur Luft- Und Raumfahrt; AlemaniaFil: Damiani, C.. Université de Paris XI; FranciaFil: Deeg, H. J.. Universidad de la Laguna; EspañaFil: Deleuil, M.. Laboratoire D; FranciaFil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Erikson, A.. Deutsches Zentrum Fur Luft- Und Raumfahrt; AlemaniaFil: Fridlund, M.. Leiden Observatory Research Institute; Países BajosFil: Gandolfi, D.. Università di Torino; ItaliaFil: Guenther, E.. Thüringer Landessternwarte; AlemaniaFil: Guillot, T.. Observatoire de la Cote D; FranciaFil: Hatzes, A.. Thüringer Landessternwarte; AlemaniaFil: Izidoro, A.. Unesp-universidade Estadual Paulista; BrasilFil: Lovis, C.. Universidad de Ginebra; SuizaFil: Moutou, C.. Laboratoire D; FranciaFil: Ollivier, M.. Université de Paris XI; FranciaFil: Pätzold, M.. Universitat Zu Köln; AlemaniaFil: Rauer, H.. Technishe Universitat Berlin; AlemaniaFil: Rouan, D.. Lesia - Laboratoire D; FranciaFil: Santerne, A.. Aix Marseille Université; FranciaFil: Schneider, J.. Université Paris Diderot - Paris 7; FranciaEDP Sciences2017-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/23612Bonomo, A. S.; Hébrard, G.; Raymond, S. N.; Bouchy, F.; Lecavelier Des Etangs, A.; et al.; A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering; EDP Sciences; Astronomy and Astrophysics; 603; A43; 7-2017; 1-110004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201730624info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2017/07/aa30624-17/aa30624-17.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:53:36Zoai:ri.conicet.gov.ar:11336/23612instacron: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 09:53:36.605CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering |
title |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering |
spellingShingle |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering Bonomo, A. S. PLANETARY SYSTEMS STARS: INDIVIDUAL: COROT-9 TECHNIQUES: PHOTOMETRIC TECHNIQUES: RADIAL VELOCITIES |
title_short |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering |
title_full |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering |
title_fullStr |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering |
title_full_unstemmed |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering |
title_sort |
A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering |
dc.creator.none.fl_str_mv |
Bonomo, A. S. Hébrard, G. Raymond, S. N. Bouchy, F. Lecavelier Des Etangs, A. Bordé, P. Aigrain, S. Almenara, J. M. Alonso, R. Cabrera, J. Csizmadia, Sz. Damiani, C. Deeg, H. J. Deleuil, M. Diaz, Rodrigo Fernando Erikson, A. Fridlund, M. Gandolfi, D. Guenther, E. Guillot, T. Hatzes, A. Izidoro, A. Lovis, C. Moutou, C. Ollivier, M. Pätzold, M. Rauer, H. Rouan, D. Santerne, A. Schneider, J. |
author |
Bonomo, A. S. |
author_facet |
Bonomo, A. S. Hébrard, G. Raymond, S. N. Bouchy, F. Lecavelier Des Etangs, A. Bordé, P. Aigrain, S. Almenara, J. M. Alonso, R. Cabrera, J. Csizmadia, Sz. Damiani, C. Deeg, H. J. Deleuil, M. Diaz, Rodrigo Fernando Erikson, A. Fridlund, M. Gandolfi, D. Guenther, E. Guillot, T. Hatzes, A. Izidoro, A. Lovis, C. Moutou, C. Ollivier, M. Pätzold, M. Rauer, H. Rouan, D. Santerne, A. Schneider, J. |
author_role |
author |
author2 |
Hébrard, G. Raymond, S. N. Bouchy, F. Lecavelier Des Etangs, A. Bordé, P. Aigrain, S. Almenara, J. M. Alonso, R. Cabrera, J. Csizmadia, Sz. Damiani, C. Deeg, H. J. Deleuil, M. Diaz, Rodrigo Fernando Erikson, A. Fridlund, M. Gandolfi, D. Guenther, E. Guillot, T. Hatzes, A. Izidoro, A. Lovis, C. Moutou, C. Ollivier, M. Pätzold, M. Rauer, H. Rouan, D. Santerne, A. Schneider, J. |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
PLANETARY SYSTEMS STARS: INDIVIDUAL: COROT-9 TECHNIQUES: PHOTOMETRIC TECHNIQUES: RADIAL VELOCITIES |
topic |
PLANETARY SYSTEMS STARS: INDIVIDUAL: COROT-9 TECHNIQUES: PHOTOMETRIC TECHNIQUES: RADIAL VELOCITIES |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
CoRoT-9b is one of the rare long-period (P = 95.3 days) transiting giant planets with a measured mass known to date. We present a new analysis of the CoRoT-9 system based on five years of radial-velocity (RV) monitoring with HARPS and three new space-based transits observed with CoRoT and Spitzer. Combining our new data with already published measurements we redetermine the CoRoT-9 system parameters and find good agreement with the published values. We uncover a higher significance for the small but non-zero eccentricity of CoRoT-9b () and find no evidence for additional planets in the system. We use simulations of planet-planet scattering to show that the eccentricity of CoRoT-9b may have been generated by an instability in which a ∼ 50 M⊕ planet was ejected from the system. This scattering would not have produced a spin-orbit misalignment, so we predict that the CoRoT-9b orbit should lie within a few degrees of the initial plane of the protoplanetary disk. As a consequence, any significant stellar obliquity would indicate that the disk was primordially tilted. Fil: Bonomo, A. S.. Istituto Nazionale Di Astrofisica; Italia Fil: Hébrard, G.. Universite de Paris I Pantheon - Sorbonne; Francia Fil: Raymond, S. N.. Laboratoire D; Francia Fil: Bouchy, F.. Universidad de Ginebra; Suiza Fil: Lecavelier Des Etangs, A.. Universite de Paris I Pantheon - Sorbonne; Francia Fil: Bordé, P.. Laboratoire D; Francia Fil: Aigrain, S.. University of Oxford; Reino Unido Fil: Almenara, J. M.. Universidad de Ginebra; Suiza Fil: Alonso, R.. Universidad de la Laguna; España Fil: Cabrera, J.. Deutsches Zentrum Fur Luft- Und Raumfahrt; Alemania Fil: Csizmadia, Sz.. Deutsches Zentrum Fur Luft- Und Raumfahrt; Alemania Fil: Damiani, C.. Université de Paris XI; Francia Fil: Deeg, H. J.. Universidad de la Laguna; España Fil: Deleuil, M.. Laboratoire D; Francia Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Erikson, A.. Deutsches Zentrum Fur Luft- Und Raumfahrt; Alemania Fil: Fridlund, M.. Leiden Observatory Research Institute; Países Bajos Fil: Gandolfi, D.. Università di Torino; Italia Fil: Guenther, E.. Thüringer Landessternwarte; Alemania Fil: Guillot, T.. Observatoire de la Cote D; Francia Fil: Hatzes, A.. Thüringer Landessternwarte; Alemania Fil: Izidoro, A.. Unesp-universidade Estadual Paulista; Brasil Fil: Lovis, C.. Universidad de Ginebra; Suiza Fil: Moutou, C.. Laboratoire D; Francia Fil: Ollivier, M.. Université de Paris XI; Francia Fil: Pätzold, M.. Universitat Zu Köln; Alemania Fil: Rauer, H.. Technishe Universitat Berlin; Alemania Fil: Rouan, D.. Lesia - Laboratoire D; Francia Fil: Santerne, A.. Aix Marseille Université; Francia Fil: Schneider, J.. Université Paris Diderot - Paris 7; Francia |
description |
CoRoT-9b is one of the rare long-period (P = 95.3 days) transiting giant planets with a measured mass known to date. We present a new analysis of the CoRoT-9 system based on five years of radial-velocity (RV) monitoring with HARPS and three new space-based transits observed with CoRoT and Spitzer. Combining our new data with already published measurements we redetermine the CoRoT-9 system parameters and find good agreement with the published values. We uncover a higher significance for the small but non-zero eccentricity of CoRoT-9b () and find no evidence for additional planets in the system. We use simulations of planet-planet scattering to show that the eccentricity of CoRoT-9b may have been generated by an instability in which a ∼ 50 M⊕ planet was ejected from the system. This scattering would not have produced a spin-orbit misalignment, so we predict that the CoRoT-9b orbit should lie within a few degrees of the initial plane of the protoplanetary disk. As a consequence, any significant stellar obliquity would indicate that the disk was primordially tilted. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-07 |
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/11336/23612 Bonomo, A. S.; Hébrard, G.; Raymond, S. N.; Bouchy, F.; Lecavelier Des Etangs, A.; et al.; A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering; EDP Sciences; Astronomy and Astrophysics; 603; A43; 7-2017; 1-11 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/23612 |
identifier_str_mv |
Bonomo, A. S.; Hébrard, G.; Raymond, S. N.; Bouchy, F.; Lecavelier Des Etangs, A.; et al.; A deeper view of the CoRoT-9 planetary system: A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering; EDP Sciences; Astronomy and Astrophysics; 603; A43; 7-2017; 1-11 0004-6361 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201730624 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2017/07/aa30624-17/aa30624-17.html |
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 |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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1844613636049338368 |
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13.070432 |