GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec
- Autores
- Pozuelos, F. J.; Suárez, J. C.; de Elía, G. C.; Berdiñas, Z.; Bonfanti, A.; Dugaro, Agustin; Guillon, M.; Jehin, E.; Mantilla Alarcon, Gunther Alfredo; Abad Santos, Natalia Vanesa; Garcia, Lorena Claudia; Thuillier, A.; Delrez, L.; Rodón, Julieta Stefanía
- Año de publicación
- 2020
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. Planets orbiting low-mass stars such as M dwarfs are now considered a cornerstone in the search for planets with thepotential to harbour life. GJ 273 is a planetary system orbiting an M dwarf only 3.75 pc away, which is composed of two confirmedplanets, GJ 273b and GJ 273c, and two promising candidates, GJ 273d and GJ 273e. Planet GJ 273b resides in the habitable zone.Currently, due to a lack of observed planetary transits, only the minimum masses of the planets are known: Mb sin ib=2.89 M⊕ ,Mc sin ic =1.18 M⊕, Md sin id =10.80 M⊕ , and Me sin ie =9.30 M⊕ . Despite its interesting character, the GJ 273 planetary system hasbeen poorly studied thus far.Aims. We aim to precisely determine the physical parameters of the individual planets, in particular, to break the mass?inclinationdegeneracy to accurately determine the mass of the planets. Moreover, we present a thorough characterisation of planet GJ 273b interms of its potential habitability.Methods. First, we explored the planetary formation and hydration phases of GJ 273 during the first 100 Myr. Secondly, we analysedthe stability of the system by considering both the two- and four-planet configurations. We then performed a comparative analysisbetween GJ 273 and the Solar System and we searched for regions in GJ 273 which may harbour minor bodies in stable orbits, that is,the main asteroid belt and Kuiper belt analogues.Results. From our set of dynamical studies, we find that the four-planet configuration of the system allows us to break the mass?inclination degeneracy. From our modelling results, the masses of the planets are unveiled as: 2.89 ≤ Mb ≤ 3.03 M⊕ , 1.18 ≤ Mc ≤1.24 M⊕ , 10.80 ≤ Md ≤ 11.35 M⊕ , and 9.30 ≤ Me ≤ 9.70 M⊕. These results point to a system that is likely to be composed of anEarth-mass planet, a super-Earth and two mini-Neptunes. Based on planetary formation models, we determine that GJ 273b is likelyan efficient water captor while GJ 273c is probably a dry planet. We find that the system may have several stable regions where minorbodies might reside. Collectively, these results are used to offer a comprehensive discussion about the habitability of GJ 273b.
Fil: Pozuelos, F. J.. Université de Liège; Bélgica
Fil: Suárez, J. C.. Universidad de Granada; España
Fil: de Elía, G. C.. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Conicet - Instituto de Astrofisica La Plata - UNLP; Argentina
Fil: Berdiñas, Z.. Universidad de Chile; Chile
Fil: Bonfanti, A.. Université de Liège; Bélgica
Fil: Dugaro, Agustin. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Guillon, M.. Université de Liège; Bélgica
Fil: Jehin, E.. Université de Liège; Bélgica
Fil: Mantilla Alarcon, Gunther Alfredo. Massachusetts Institute Of Technology; Estados Unidos
Fil: Abad Santos, Natalia Vanesa. Université de Liège; Bélgica
Fil: Garcia, Lorena Claudia. Université de Liège; Bélgica
Fil: Thuillier, A.. Université de Liège; Bélgica
Fil: Delrez, L.. Université de Liège; Bélgica
Fil: Rodón, Julieta Stefanía. Instituto de Astrofísica de Andalucía; España - Materia
-
PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY
PLANETS AND SATELLITES: FORMATION - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/145851
Ver los metadatos del registro completo
| id |
CONICETDig_7936a133bb52c29b4c0e2740cfcf75d8 |
|---|---|
| oai_identifier_str |
oai:ri.conicet.gov.ar:11336/145851 |
| network_acronym_str |
CONICETDig |
| repository_id_str |
3498 |
| network_name_str |
CONICET Digital (CONICET) |
| spelling |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsecPozuelos, F. J.Suárez, J. C.de Elía, G. C.Berdiñas, Z.Bonfanti, A.Dugaro, AgustinGuillon, M.Jehin, E.Mantilla Alarcon, Gunther AlfredoAbad Santos, Natalia VanesaGarcia, Lorena ClaudiaThuillier, A.Delrez, L.Rodón, Julieta StefaníaPLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITYPLANETS AND SATELLITES: FORMATIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. Planets orbiting low-mass stars such as M dwarfs are now considered a cornerstone in the search for planets with thepotential to harbour life. GJ 273 is a planetary system orbiting an M dwarf only 3.75 pc away, which is composed of two confirmedplanets, GJ 273b and GJ 273c, and two promising candidates, GJ 273d and GJ 273e. Planet GJ 273b resides in the habitable zone.Currently, due to a lack of observed planetary transits, only the minimum masses of the planets are known: Mb sin ib=2.89 M⊕ ,Mc sin ic =1.18 M⊕, Md sin id =10.80 M⊕ , and Me sin ie =9.30 M⊕ . Despite its interesting character, the GJ 273 planetary system hasbeen poorly studied thus far.Aims. We aim to precisely determine the physical parameters of the individual planets, in particular, to break the mass?inclinationdegeneracy to accurately determine the mass of the planets. Moreover, we present a thorough characterisation of planet GJ 273b interms of its potential habitability.Methods. First, we explored the planetary formation and hydration phases of GJ 273 during the first 100 Myr. Secondly, we analysedthe stability of the system by considering both the two- and four-planet configurations. We then performed a comparative analysisbetween GJ 273 and the Solar System and we searched for regions in GJ 273 which may harbour minor bodies in stable orbits, that is,the main asteroid belt and Kuiper belt analogues.Results. From our set of dynamical studies, we find that the four-planet configuration of the system allows us to break the mass?inclination degeneracy. From our modelling results, the masses of the planets are unveiled as: 2.89 ≤ Mb ≤ 3.03 M⊕ , 1.18 ≤ Mc ≤1.24 M⊕ , 10.80 ≤ Md ≤ 11.35 M⊕ , and 9.30 ≤ Me ≤ 9.70 M⊕. These results point to a system that is likely to be composed of anEarth-mass planet, a super-Earth and two mini-Neptunes. Based on planetary formation models, we determine that GJ 273b is likelyan efficient water captor while GJ 273c is probably a dry planet. We find that the system may have several stable regions where minorbodies might reside. Collectively, these results are used to offer a comprehensive discussion about the habitability of GJ 273b.Fil: Pozuelos, F. J.. Université de Liège; BélgicaFil: Suárez, J. C.. Universidad de Granada; EspañaFil: de Elía, G. C.. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Conicet - Instituto de Astrofisica La Plata - UNLP; ArgentinaFil: Berdiñas, Z.. Universidad de Chile; ChileFil: Bonfanti, A.. Université de Liège; BélgicaFil: Dugaro, Agustin. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Guillon, M.. Université de Liège; BélgicaFil: Jehin, E.. Université de Liège; BélgicaFil: Mantilla Alarcon, Gunther Alfredo. Massachusetts Institute Of Technology; Estados UnidosFil: Abad Santos, Natalia Vanesa. Université de Liège; BélgicaFil: Garcia, Lorena Claudia. Université de Liège; BélgicaFil: Thuillier, A.. Université de Liège; BélgicaFil: Delrez, L.. Université de Liège; BélgicaFil: Rodón, Julieta Stefanía. Instituto de Astrofísica de Andalucía; EspañaEDP Sciences2020-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/zipapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/145851Pozuelos, F. J.; Suárez, J. C.; de Elía, G. C.; Berdiñas, Z.; Bonfanti, A.; et al.; GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec; EDP Sciences; Astronomy and Astrophysics; 641; A23; 9-2020; 1-190004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202038047info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2006.09403info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:47:09Zoai:ri.conicet.gov.ar:11336/145851instacron: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 09:47:10.199CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec |
| title |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec |
| spellingShingle |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec Pozuelos, F. J. PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY PLANETS AND SATELLITES: FORMATION |
| title_short |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec |
| title_full |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec |
| title_fullStr |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec |
| title_full_unstemmed |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec |
| title_sort |
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec |
| dc.creator.none.fl_str_mv |
Pozuelos, F. J. Suárez, J. C. de Elía, G. C. Berdiñas, Z. Bonfanti, A. Dugaro, Agustin Guillon, M. Jehin, E. Mantilla Alarcon, Gunther Alfredo Abad Santos, Natalia Vanesa Garcia, Lorena Claudia Thuillier, A. Delrez, L. Rodón, Julieta Stefanía |
| author |
Pozuelos, F. J. |
| author_facet |
Pozuelos, F. J. Suárez, J. C. de Elía, G. C. Berdiñas, Z. Bonfanti, A. Dugaro, Agustin Guillon, M. Jehin, E. Mantilla Alarcon, Gunther Alfredo Abad Santos, Natalia Vanesa Garcia, Lorena Claudia Thuillier, A. Delrez, L. Rodón, Julieta Stefanía |
| author_role |
author |
| author2 |
Suárez, J. C. de Elía, G. C. Berdiñas, Z. Bonfanti, A. Dugaro, Agustin Guillon, M. Jehin, E. Mantilla Alarcon, Gunther Alfredo Abad Santos, Natalia Vanesa Garcia, Lorena Claudia Thuillier, A. Delrez, L. Rodón, Julieta Stefanía |
| author2_role |
author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY PLANETS AND SATELLITES: FORMATION |
| topic |
PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY PLANETS AND SATELLITES: FORMATION |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Context. Planets orbiting low-mass stars such as M dwarfs are now considered a cornerstone in the search for planets with thepotential to harbour life. GJ 273 is a planetary system orbiting an M dwarf only 3.75 pc away, which is composed of two confirmedplanets, GJ 273b and GJ 273c, and two promising candidates, GJ 273d and GJ 273e. Planet GJ 273b resides in the habitable zone.Currently, due to a lack of observed planetary transits, only the minimum masses of the planets are known: Mb sin ib=2.89 M⊕ ,Mc sin ic =1.18 M⊕, Md sin id =10.80 M⊕ , and Me sin ie =9.30 M⊕ . Despite its interesting character, the GJ 273 planetary system hasbeen poorly studied thus far.Aims. We aim to precisely determine the physical parameters of the individual planets, in particular, to break the mass?inclinationdegeneracy to accurately determine the mass of the planets. Moreover, we present a thorough characterisation of planet GJ 273b interms of its potential habitability.Methods. First, we explored the planetary formation and hydration phases of GJ 273 during the first 100 Myr. Secondly, we analysedthe stability of the system by considering both the two- and four-planet configurations. We then performed a comparative analysisbetween GJ 273 and the Solar System and we searched for regions in GJ 273 which may harbour minor bodies in stable orbits, that is,the main asteroid belt and Kuiper belt analogues.Results. From our set of dynamical studies, we find that the four-planet configuration of the system allows us to break the mass?inclination degeneracy. From our modelling results, the masses of the planets are unveiled as: 2.89 ≤ Mb ≤ 3.03 M⊕ , 1.18 ≤ Mc ≤1.24 M⊕ , 10.80 ≤ Md ≤ 11.35 M⊕ , and 9.30 ≤ Me ≤ 9.70 M⊕. These results point to a system that is likely to be composed of anEarth-mass planet, a super-Earth and two mini-Neptunes. Based on planetary formation models, we determine that GJ 273b is likelyan efficient water captor while GJ 273c is probably a dry planet. We find that the system may have several stable regions where minorbodies might reside. Collectively, these results are used to offer a comprehensive discussion about the habitability of GJ 273b. Fil: Pozuelos, F. J.. Université de Liège; Bélgica Fil: Suárez, J. C.. Universidad de Granada; España Fil: de Elía, G. C.. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Conicet - Instituto de Astrofisica La Plata - UNLP; Argentina Fil: Berdiñas, Z.. Universidad de Chile; Chile Fil: Bonfanti, A.. Université de Liège; Bélgica Fil: Dugaro, Agustin. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Guillon, M.. Université de Liège; Bélgica Fil: Jehin, E.. Université de Liège; Bélgica Fil: Mantilla Alarcon, Gunther Alfredo. Massachusetts Institute Of Technology; Estados Unidos Fil: Abad Santos, Natalia Vanesa. Université de Liège; Bélgica Fil: Garcia, Lorena Claudia. Université de Liège; Bélgica Fil: Thuillier, A.. Université de Liège; Bélgica Fil: Delrez, L.. Université de Liège; Bélgica Fil: Rodón, Julieta Stefanía. Instituto de Astrofísica de Andalucía; España |
| description |
Context. Planets orbiting low-mass stars such as M dwarfs are now considered a cornerstone in the search for planets with thepotential to harbour life. GJ 273 is a planetary system orbiting an M dwarf only 3.75 pc away, which is composed of two confirmedplanets, GJ 273b and GJ 273c, and two promising candidates, GJ 273d and GJ 273e. Planet GJ 273b resides in the habitable zone.Currently, due to a lack of observed planetary transits, only the minimum masses of the planets are known: Mb sin ib=2.89 M⊕ ,Mc sin ic =1.18 M⊕, Md sin id =10.80 M⊕ , and Me sin ie =9.30 M⊕ . Despite its interesting character, the GJ 273 planetary system hasbeen poorly studied thus far.Aims. We aim to precisely determine the physical parameters of the individual planets, in particular, to break the mass?inclinationdegeneracy to accurately determine the mass of the planets. Moreover, we present a thorough characterisation of planet GJ 273b interms of its potential habitability.Methods. First, we explored the planetary formation and hydration phases of GJ 273 during the first 100 Myr. Secondly, we analysedthe stability of the system by considering both the two- and four-planet configurations. We then performed a comparative analysisbetween GJ 273 and the Solar System and we searched for regions in GJ 273 which may harbour minor bodies in stable orbits, that is,the main asteroid belt and Kuiper belt analogues.Results. From our set of dynamical studies, we find that the four-planet configuration of the system allows us to break the mass?inclination degeneracy. From our modelling results, the masses of the planets are unveiled as: 2.89 ≤ Mb ≤ 3.03 M⊕ , 1.18 ≤ Mc ≤1.24 M⊕ , 10.80 ≤ Md ≤ 11.35 M⊕ , and 9.30 ≤ Me ≤ 9.70 M⊕. These results point to a system that is likely to be composed of anEarth-mass planet, a super-Earth and two mini-Neptunes. Based on planetary formation models, we determine that GJ 273b is likelyan efficient water captor while GJ 273c is probably a dry planet. We find that the system may have several stable regions where minorbodies might reside. Collectively, these results are used to offer a comprehensive discussion about the habitability of GJ 273b. |
| publishDate |
2020 |
| dc.date.none.fl_str_mv |
2020-09 |
| 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/11336/145851 Pozuelos, F. J.; Suárez, J. C.; de Elía, G. C.; Berdiñas, Z.; Bonfanti, A.; et al.; GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec; EDP Sciences; Astronomy and Astrophysics; 641; A23; 9-2020; 1-19 0004-6361 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/145851 |
| identifier_str_mv |
Pozuelos, F. J.; Suárez, J. C.; de Elía, G. C.; Berdiñas, Z.; Bonfanti, A.; et al.; GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec; EDP Sciences; Astronomy and Astrophysics; 641; A23; 9-2020; 1-19 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/10.1051/0004-6361/202038047 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2006.09403 |
| 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/zip 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) |
| 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_ |
1844613470123720704 |
| score |
13.070432 |