A temperate exo-Earth around a quiet M dwarf at 3.4 parsec
- Autores
- Bonfils, X.; Astudillo Defru, Nicola; Diaz, Rodrigo Fernando; Almenara, J.-M.; Forveille, T.; Bouchy, F.; Delfosse, X.; Lovis, C.; Mayor, M.; Murgas, F.; Pepe, F.; Santos, N.C.; Ségransan, D.; Udry, S.; Wünsche, A.
- Año de publicación
- 2018
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The combination of high-contrast imaging and high-dispersion spectroscopy, which has successfully been use to detect the atmosphere of a giant planet, is one of the most promising potential probes of the atmosphere of Earth-size worlds. The forthcoming generation of extremely large telescopes (ELTs) may obtain sufficient contrast with this technique to detect O2 in the atmosphere of those worlds that orbit low-mass M dwarfs. This is strong motivation to carry out a census of planets around cool stars for which habitable zones can be resolved by ELTs, i.e. for M dwarfs within ~5 parsec. Our HARPS survey has been a major contributor to that sample of nearby planets. Here we report on our radial velocity observations of Ross 128 (Proxima Virginis, GJ447, HIP 57548), an M4 dwarf just 3.4 parsec away from our Sun. This source hosts an exo-Earth with a projected mass m sini = 1.35 M and an orbital period of 9.9 days. Ross 128 b receives less than 1.5 times as much flux as Earth from the Sun and its equilibrium ranges in temperature between 269 K for an Earth-like albedo and 213 K for a Venus-like albedo. Recent studies place it close to the inner edge of the conventional habitable zone. An 80-day long light curve from K2 campaign C01 demonstrates that Ross 128 b does not transit. Together with the All Sky Automated Survey (ASAS) photometry and spectroscopic activity indices, the K2 photometry shows that Ross 128 rotates slowly and has weak magnetic activity. In a habitability context, this makes survival of its atmosphere against erosion more likely. Ross 128 b is the second closest known exo-Earth, after Proxima Centauri b (1.3 parsec), and the closest temperate planet known around a quiet star. The 15 mas planet-star angular separation at maximum elongation will be resolved by ELTs (>3λD) in the optical bands of O2.
Fil: Bonfils, X.. Universite Grenoble Alpes; Francia
Fil: Astudillo Defru, Nicola. Universidad de Ginebra; Suiza
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. Universidad de Buenos Aires; Argentina
Fil: Almenara, J.-M.. Universidad de Ginebra; Suiza
Fil: Forveille, T.. Universite Grenoble Alpes; Francia
Fil: Bouchy, F.. Universidad de Ginebra; Suiza
Fil: Delfosse, X.. Universite Grenoble Alpes; Francia
Fil: Lovis, C.. Universidad de Ginebra; Suiza
Fil: Mayor, M.. Universidad de Ginebra; Suiza
Fil: Murgas, F.. Instituto Astrofisico de Canarias; España. Universidad de La Laguna; España
Fil: Pepe, F.. Universidad de Ginebra; Suiza
Fil: Santos, N.C.. Universidad de Porto; Portugal
Fil: Ségransan, D.. Universidad de Ginebra; Suiza
Fil: Udry, S.. Universidad de Ginebra; Suiza
Fil: Wünsche, A.. Universite Grenoble Alpes; Francia - Materia
-
PLANETARY SYSTEMS
STARS: LATE-TYPE
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:11336/209352
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A temperate exo-Earth around a quiet M dwarf at 3.4 parsecBonfils, X.Astudillo Defru, NicolaDiaz, Rodrigo FernandoAlmenara, J.-M.Forveille, T.Bouchy, F.Delfosse, X.Lovis, C.Mayor, M.Murgas, F.Pepe, F.Santos, N.C.Ségransan, D.Udry, S.Wünsche, A.PLANETARY SYSTEMSSTARS: LATE-TYPETECHNIQUES: RADIAL VELOCITIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The combination of high-contrast imaging and high-dispersion spectroscopy, which has successfully been use to detect the atmosphere of a giant planet, is one of the most promising potential probes of the atmosphere of Earth-size worlds. The forthcoming generation of extremely large telescopes (ELTs) may obtain sufficient contrast with this technique to detect O2 in the atmosphere of those worlds that orbit low-mass M dwarfs. This is strong motivation to carry out a census of planets around cool stars for which habitable zones can be resolved by ELTs, i.e. for M dwarfs within ~5 parsec. Our HARPS survey has been a major contributor to that sample of nearby planets. Here we report on our radial velocity observations of Ross 128 (Proxima Virginis, GJ447, HIP 57548), an M4 dwarf just 3.4 parsec away from our Sun. This source hosts an exo-Earth with a projected mass m sini = 1.35 M and an orbital period of 9.9 days. Ross 128 b receives less than 1.5 times as much flux as Earth from the Sun and its equilibrium ranges in temperature between 269 K for an Earth-like albedo and 213 K for a Venus-like albedo. Recent studies place it close to the inner edge of the conventional habitable zone. An 80-day long light curve from K2 campaign C01 demonstrates that Ross 128 b does not transit. Together with the All Sky Automated Survey (ASAS) photometry and spectroscopic activity indices, the K2 photometry shows that Ross 128 rotates slowly and has weak magnetic activity. In a habitability context, this makes survival of its atmosphere against erosion more likely. Ross 128 b is the second closest known exo-Earth, after Proxima Centauri b (1.3 parsec), and the closest temperate planet known around a quiet star. The 15 mas planet-star angular separation at maximum elongation will be resolved by ELTs (>3λD) in the optical bands of O2.Fil: Bonfils, X.. Universite Grenoble Alpes; FranciaFil: Astudillo Defru, Nicola. Universidad de Ginebra; SuizaFil: 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. Universidad de Buenos Aires; ArgentinaFil: Almenara, J.-M.. Universidad de Ginebra; SuizaFil: Forveille, T.. Universite Grenoble Alpes; FranciaFil: Bouchy, F.. Universidad de Ginebra; SuizaFil: Delfosse, X.. Universite Grenoble Alpes; FranciaFil: Lovis, C.. Universidad de Ginebra; SuizaFil: Mayor, M.. Universidad de Ginebra; SuizaFil: Murgas, F.. Instituto Astrofisico de Canarias; España. Universidad de La Laguna; EspañaFil: Pepe, F.. Universidad de Ginebra; SuizaFil: Santos, N.C.. Universidad de Porto; PortugalFil: Ségransan, D.. Universidad de Ginebra; SuizaFil: Udry, S.. Universidad de Ginebra; SuizaFil: Wünsche, A.. Universite Grenoble Alpes; FranciaEDP Sciences2018-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/209352Bonfils, X.; Astudillo Defru, Nicola; Diaz, Rodrigo Fernando; Almenara, J.-M.; Forveille, T.; et al.; A temperate exo-Earth around a quiet M dwarf at 3.4 parsec; EDP Sciences; Astronomy and Astrophysics; 613; A25; 5-2018; 1-90004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201731973info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2018/05/aa31973-17/aa31973-17.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 Técnicas2025-09-29T09:43:01Zoai:ri.conicet.gov.ar:11336/209352instacron: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 09:43:01.578CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec |
title |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec |
spellingShingle |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec Bonfils, X. PLANETARY SYSTEMS STARS: LATE-TYPE TECHNIQUES: RADIAL VELOCITIES |
title_short |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec |
title_full |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec |
title_fullStr |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec |
title_full_unstemmed |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec |
title_sort |
A temperate exo-Earth around a quiet M dwarf at 3.4 parsec |
dc.creator.none.fl_str_mv |
Bonfils, X. Astudillo Defru, Nicola Diaz, Rodrigo Fernando Almenara, J.-M. Forveille, T. Bouchy, F. Delfosse, X. Lovis, C. Mayor, M. Murgas, F. Pepe, F. Santos, N.C. Ségransan, D. Udry, S. Wünsche, A. |
author |
Bonfils, X. |
author_facet |
Bonfils, X. Astudillo Defru, Nicola Diaz, Rodrigo Fernando Almenara, J.-M. Forveille, T. Bouchy, F. Delfosse, X. Lovis, C. Mayor, M. Murgas, F. Pepe, F. Santos, N.C. Ségransan, D. Udry, S. Wünsche, A. |
author_role |
author |
author2 |
Astudillo Defru, Nicola Diaz, Rodrigo Fernando Almenara, J.-M. Forveille, T. Bouchy, F. Delfosse, X. Lovis, C. Mayor, M. Murgas, F. Pepe, F. Santos, N.C. Ségransan, D. Udry, S. Wünsche, A. |
author2_role |
author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
PLANETARY SYSTEMS STARS: LATE-TYPE TECHNIQUES: RADIAL VELOCITIES |
topic |
PLANETARY SYSTEMS STARS: LATE-TYPE 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 |
The combination of high-contrast imaging and high-dispersion spectroscopy, which has successfully been use to detect the atmosphere of a giant planet, is one of the most promising potential probes of the atmosphere of Earth-size worlds. The forthcoming generation of extremely large telescopes (ELTs) may obtain sufficient contrast with this technique to detect O2 in the atmosphere of those worlds that orbit low-mass M dwarfs. This is strong motivation to carry out a census of planets around cool stars for which habitable zones can be resolved by ELTs, i.e. for M dwarfs within ~5 parsec. Our HARPS survey has been a major contributor to that sample of nearby planets. Here we report on our radial velocity observations of Ross 128 (Proxima Virginis, GJ447, HIP 57548), an M4 dwarf just 3.4 parsec away from our Sun. This source hosts an exo-Earth with a projected mass m sini = 1.35 M and an orbital period of 9.9 days. Ross 128 b receives less than 1.5 times as much flux as Earth from the Sun and its equilibrium ranges in temperature between 269 K for an Earth-like albedo and 213 K for a Venus-like albedo. Recent studies place it close to the inner edge of the conventional habitable zone. An 80-day long light curve from K2 campaign C01 demonstrates that Ross 128 b does not transit. Together with the All Sky Automated Survey (ASAS) photometry and spectroscopic activity indices, the K2 photometry shows that Ross 128 rotates slowly and has weak magnetic activity. In a habitability context, this makes survival of its atmosphere against erosion more likely. Ross 128 b is the second closest known exo-Earth, after Proxima Centauri b (1.3 parsec), and the closest temperate planet known around a quiet star. The 15 mas planet-star angular separation at maximum elongation will be resolved by ELTs (>3λD) in the optical bands of O2. Fil: Bonfils, X.. Universite Grenoble Alpes; Francia Fil: Astudillo Defru, Nicola. Universidad de Ginebra; Suiza 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. Universidad de Buenos Aires; Argentina Fil: Almenara, J.-M.. Universidad de Ginebra; Suiza Fil: Forveille, T.. Universite Grenoble Alpes; Francia Fil: Bouchy, F.. Universidad de Ginebra; Suiza Fil: Delfosse, X.. Universite Grenoble Alpes; Francia Fil: Lovis, C.. Universidad de Ginebra; Suiza Fil: Mayor, M.. Universidad de Ginebra; Suiza Fil: Murgas, F.. Instituto Astrofisico de Canarias; España. Universidad de La Laguna; España Fil: Pepe, F.. Universidad de Ginebra; Suiza Fil: Santos, N.C.. Universidad de Porto; Portugal Fil: Ségransan, D.. Universidad de Ginebra; Suiza Fil: Udry, S.. Universidad de Ginebra; Suiza Fil: Wünsche, A.. Universite Grenoble Alpes; Francia |
description |
The combination of high-contrast imaging and high-dispersion spectroscopy, which has successfully been use to detect the atmosphere of a giant planet, is one of the most promising potential probes of the atmosphere of Earth-size worlds. The forthcoming generation of extremely large telescopes (ELTs) may obtain sufficient contrast with this technique to detect O2 in the atmosphere of those worlds that orbit low-mass M dwarfs. This is strong motivation to carry out a census of planets around cool stars for which habitable zones can be resolved by ELTs, i.e. for M dwarfs within ~5 parsec. Our HARPS survey has been a major contributor to that sample of nearby planets. Here we report on our radial velocity observations of Ross 128 (Proxima Virginis, GJ447, HIP 57548), an M4 dwarf just 3.4 parsec away from our Sun. This source hosts an exo-Earth with a projected mass m sini = 1.35 M and an orbital period of 9.9 days. Ross 128 b receives less than 1.5 times as much flux as Earth from the Sun and its equilibrium ranges in temperature between 269 K for an Earth-like albedo and 213 K for a Venus-like albedo. Recent studies place it close to the inner edge of the conventional habitable zone. An 80-day long light curve from K2 campaign C01 demonstrates that Ross 128 b does not transit. Together with the All Sky Automated Survey (ASAS) photometry and spectroscopic activity indices, the K2 photometry shows that Ross 128 rotates slowly and has weak magnetic activity. In a habitability context, this makes survival of its atmosphere against erosion more likely. Ross 128 b is the second closest known exo-Earth, after Proxima Centauri b (1.3 parsec), and the closest temperate planet known around a quiet star. The 15 mas planet-star angular separation at maximum elongation will be resolved by ELTs (>3λD) in the optical bands of O2. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-05 |
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/11336/209352 Bonfils, X.; Astudillo Defru, Nicola; Diaz, Rodrigo Fernando; Almenara, J.-M.; Forveille, T.; et al.; A temperate exo-Earth around a quiet M dwarf at 3.4 parsec; EDP Sciences; Astronomy and Astrophysics; 613; A25; 5-2018; 1-9 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/209352 |
identifier_str_mv |
Bonfils, X.; Astudillo Defru, Nicola; Diaz, Rodrigo Fernando; Almenara, J.-M.; Forveille, T.; et al.; A temperate exo-Earth around a quiet M dwarf at 3.4 parsec; EDP Sciences; Astronomy and Astrophysics; 613; A25; 5-2018; 1-9 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/10.1051/0004-6361/201731973 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2018/05/aa31973-17/aa31973-17.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) |
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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1844613353789456384 |
score |
13.070432 |