A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS

Autores: Astudillo Defru, Nicola; Cloutier, R.; Wang, S. X.; Teske, J.; Brahm, R.; Hellier, C.; Ricker, G.; Vanderspek, R.; Latham, D.; Seager, S.; Winn, J. N.; Jenkins, J. M.; Collins, K. A.; Stassun, K. G.; Ziegler, C.; Almenara, J. M.; Anderson, D. R.; Artigau, E.; Bonfils, X.; Bouchy, F.; Briceño, C.; Butler, R. P.; Charbonneau, D.; Conti, D. M.; Crane, J.; Crossfield, I. J. M.; Davies, M.; Delfosse, X.; Diaz, Rodrigo Fernando; Doyon, R.
Año de publicación: 2020
Idioma: inglés
Tipo de recurso: artículo
Estado: versión publicada
Descripción: We report the detection of a transiting super-Earth-sized planet (R = 1.39 ± 0.09 R⊕ ) in a 1.4-day orbit around L 168-9 (TOI-134), a bright M1V dwarf (V = 11, K = 7.1) located at 25.15 ± 0.02 pc. The host star was observed in the first sector of the Transiting Exoplanet Survey Satellite (TESS) mission. For confirmation and planet mass measurement purposes, this was followed up with ground-based photometry, seeing-limited and high-resolution imaging, and precise radial velocity (PRV) observations using the HARPS and Magellan/PFS spectrographs. By combining the TESS data and PRV observations, we find the mass of L 168-9 b to be 4.60 ± 0.56 M⊕ and thus the bulk density to be 1.74-0.33+0.44 times higher than that of the Earth. The orbital eccentricity is smaller than 0.21 (95% confidence). This planet is a level one candidate for the TESS mission's scientific objective of measuring the masses of 50 small planets, and it is one of the most observationally accessible terrestrial planets for future atmospheric characterization.
Fil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; Chile
Fil: Cloutier, R.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Toronto; Canadá
Fil: Wang, S. X.. Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Teske, J.. Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Brahm, R.. Millennium Institute of Astrophysics; Chile. Pontificia Universidad Católica de Chile; Chile
Fil: Hellier, C.. Keele University; Reino Unido
Fil: Ricker, G.. Massachusetts Institute of Technology; Estados Unidos
Fil: Vanderspek, R.. Massachusetts Institute of Technology; Estados Unidos
Fil: Latham, D.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Seager, S.. Massachusetts Institute of Technology; Estados Unidos
Fil: Winn, J. N.. University of Princeton; Estados Unidos
Fil: Jenkins, J. M.. National Aeronautics and Space Administration; Estados Unidos
Fil: Collins, K. A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Stassun, K. G.. Vanderbilt University; Estados Unidos
Fil: Ziegler, C.. University of Toronto; Canadá
Fil: Almenara, J. M.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Anderson, D. R.. Keele University; Reino Unido. University of Warwick; Reino Unido
Fil: Artigau, E.. University of Montreal; Canadá
Fil: Bonfils, X.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Bouchy, F.. Universidad de Ginebra; Suiza
Fil: Briceño, C.. Cerro Tololo Inter American Observatory; Chile
Fil: Butler, R. P.. Carnegie Institution for Science; Estados Unidos
Fil: Charbonneau, D.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Conti, D. M.. American Association of Variable Star Observers; Estados Unidos
Fil: Crane, J.. Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Crossfield, I. J. M.. Massachusetts Institute of Technology; Estados Unidos. University of Kansas; Estados Unidos
Fil: Davies, M.. National Aeronautics and Space Administration; Estados Unidos
Fil: Delfosse, X.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Diaz, Rodrigo Fernando. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); Argentina
Fil: Doyon, R.. University of Montreal; Canadá
Materia: PLANETARY SYSTEMS
STARS: INDIVIDUAL: L 168-9
STARS: LATE-TYPE
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
Nivel de accesibilidad: acceso abierto
Condiciones de uso: https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
Institución: Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador: oai:ri.conicet.gov.ar:11336/151445

Acceder

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network_acronym_str	CONICETDig
repository_id_str	3498
network_name_str	CONICET Digital (CONICET)
spelling	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESSAstudillo Defru, NicolaCloutier, R.Wang, S. X.Teske, J.Brahm, R.Hellier, C.Ricker, G.Vanderspek, R.Latham, D.Seager, S.Winn, J. N.Jenkins, J. M.Collins, K. A.Stassun, K. G.Ziegler, C.Almenara, J. M.Anderson, D. R.Artigau, E.Bonfils, X.Bouchy, F.Briceño, C.Butler, R. P.Charbonneau, D.Conti, D. M.Crane, J.Crossfield, I. J. M.Davies, M.Delfosse, X.Diaz, Rodrigo FernandoDoyon, R.PLANETARY SYSTEMSSTARS: INDIVIDUAL: L 168-9STARS: LATE-TYPETECHNIQUES: PHOTOMETRICTECHNIQUES: RADIAL VELOCITIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We report the detection of a transiting super-Earth-sized planet (R = 1.39 ± 0.09 R⊕ ) in a 1.4-day orbit around L 168-9 (TOI-134), a bright M1V dwarf (V = 11, K = 7.1) located at 25.15 ± 0.02 pc. The host star was observed in the first sector of the Transiting Exoplanet Survey Satellite (TESS) mission. For confirmation and planet mass measurement purposes, this was followed up with ground-based photometry, seeing-limited and high-resolution imaging, and precise radial velocity (PRV) observations using the HARPS and Magellan/PFS spectrographs. By combining the TESS data and PRV observations, we find the mass of L 168-9 b to be 4.60 ± 0.56 M⊕ and thus the bulk density to be 1.74-0.33+0.44 times higher than that of the Earth. The orbital eccentricity is smaller than 0.21 (95% confidence). This planet is a level one candidate for the TESS mission's scientific objective of measuring the masses of 50 small planets, and it is one of the most observationally accessible terrestrial planets for future atmospheric characterization.Fil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; ChileFil: Cloutier, R.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Toronto; CanadáFil: Wang, S. X.. Observatories of the Carnegie Institution for Science; Estados UnidosFil: Teske, J.. Observatories of the Carnegie Institution for Science; Estados UnidosFil: Brahm, R.. Millennium Institute of Astrophysics; Chile. Pontificia Universidad Católica de Chile; ChileFil: Hellier, C.. Keele University; Reino UnidoFil: Ricker, G.. Massachusetts Institute of Technology; Estados UnidosFil: Vanderspek, R.. Massachusetts Institute of Technology; Estados UnidosFil: Latham, D.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Seager, S.. Massachusetts Institute of Technology; Estados UnidosFil: Winn, J. N.. University of Princeton; Estados UnidosFil: Jenkins, J. M.. National Aeronautics and Space Administration; Estados UnidosFil: Collins, K. A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Stassun, K. G.. Vanderbilt University; Estados UnidosFil: Ziegler, C.. University of Toronto; CanadáFil: Almenara, J. M.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; FranciaFil: Anderson, D. R.. Keele University; Reino Unido. University of Warwick; Reino UnidoFil: Artigau, E.. University of Montreal; CanadáFil: Bonfils, X.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; FranciaFil: Bouchy, F.. Universidad de Ginebra; SuizaFil: Briceño, C.. Cerro Tololo Inter American Observatory; ChileFil: Butler, R. P.. Carnegie Institution for Science; Estados UnidosFil: Charbonneau, D.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Conti, D. M.. American Association of Variable Star Observers; Estados UnidosFil: Crane, J.. Observatories of the Carnegie Institution for Science; Estados UnidosFil: Crossfield, I. J. M.. Massachusetts Institute of Technology; Estados Unidos. University of Kansas; Estados UnidosFil: Davies, M.. National Aeronautics and Space Administration; Estados UnidosFil: Delfosse, X.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; FranciaFil: Diaz, Rodrigo Fernando. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); ArgentinaFil: Doyon, R.. University of Montreal; CanadáEDP Sciences2020-04info: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/11336/151445Astudillo Defru, Nicola; Cloutier, R.; Wang, S. X.; Teske, J.; Brahm, R.; et al.; A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS; EDP Sciences; Astronomy and Astrophysics; 636; 4-2020; 1-130004-63611432-0746CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201937179info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2001.09175info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:45:03Zoai:ri.conicet.gov.ar:11336/151445instacron: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 09:45:03.471CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
title	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
spellingShingle	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS Astudillo Defru, Nicola PLANETARY SYSTEMS STARS: INDIVIDUAL: L 168-9 STARS: LATE-TYPE TECHNIQUES: PHOTOMETRIC TECHNIQUES: RADIAL VELOCITIES
title_short	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
title_full	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
title_fullStr	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
title_full_unstemmed	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
title_sort	A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
dc.creator.none.fl_str_mv	Astudillo Defru, Nicola Cloutier, R. Wang, S. X. Teske, J. Brahm, R. Hellier, C. Ricker, G. Vanderspek, R. Latham, D. Seager, S. Winn, J. N. Jenkins, J. M. Collins, K. A. Stassun, K. G. Ziegler, C. Almenara, J. M. Anderson, D. R. Artigau, E. Bonfils, X. Bouchy, F. Briceño, C. Butler, R. P. Charbonneau, D. Conti, D. M. Crane, J. Crossfield, I. J. M. Davies, M. Delfosse, X. Diaz, Rodrigo Fernando Doyon, R.
author	Astudillo Defru, Nicola
author_facet	Astudillo Defru, Nicola Cloutier, R. Wang, S. X. Teske, J. Brahm, R. Hellier, C. Ricker, G. Vanderspek, R. Latham, D. Seager, S. Winn, J. N. Jenkins, J. M. Collins, K. A. Stassun, K. G. Ziegler, C. Almenara, J. M. Anderson, D. R. Artigau, E. Bonfils, X. Bouchy, F. Briceño, C. Butler, R. P. Charbonneau, D. Conti, D. M. Crane, J. Crossfield, I. J. M. Davies, M. Delfosse, X. Diaz, Rodrigo Fernando Doyon, R.
author_role	author
author2	Cloutier, R. Wang, S. X. Teske, J. Brahm, R. Hellier, C. Ricker, G. Vanderspek, R. Latham, D. Seager, S. Winn, J. N. Jenkins, J. M. Collins, K. A. Stassun, K. G. Ziegler, C. Almenara, J. M. Anderson, D. R. Artigau, E. Bonfils, X. Bouchy, F. Briceño, C. Butler, R. P. Charbonneau, D. Conti, D. M. Crane, J. Crossfield, I. J. M. Davies, M. Delfosse, X. Diaz, Rodrigo Fernando Doyon, R.
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: L 168-9 STARS: LATE-TYPE TECHNIQUES: PHOTOMETRIC TECHNIQUES: RADIAL VELOCITIES
topic	PLANETARY SYSTEMS STARS: INDIVIDUAL: L 168-9 STARS: LATE-TYPE 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	We report the detection of a transiting super-Earth-sized planet (R = 1.39 ± 0.09 R⊕ ) in a 1.4-day orbit around L 168-9 (TOI-134), a bright M1V dwarf (V = 11, K = 7.1) located at 25.15 ± 0.02 pc. The host star was observed in the first sector of the Transiting Exoplanet Survey Satellite (TESS) mission. For confirmation and planet mass measurement purposes, this was followed up with ground-based photometry, seeing-limited and high-resolution imaging, and precise radial velocity (PRV) observations using the HARPS and Magellan/PFS spectrographs. By combining the TESS data and PRV observations, we find the mass of L 168-9 b to be 4.60 ± 0.56 M⊕ and thus the bulk density to be 1.74-0.33+0.44 times higher than that of the Earth. The orbital eccentricity is smaller than 0.21 (95% confidence). This planet is a level one candidate for the TESS mission's scientific objective of measuring the masses of 50 small planets, and it is one of the most observationally accessible terrestrial planets for future atmospheric characterization. Fil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; Chile Fil: Cloutier, R.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Toronto; Canadá Fil: Wang, S. X.. Observatories of the Carnegie Institution for Science; Estados Unidos Fil: Teske, J.. Observatories of the Carnegie Institution for Science; Estados Unidos Fil: Brahm, R.. Millennium Institute of Astrophysics; Chile. Pontificia Universidad Católica de Chile; Chile Fil: Hellier, C.. Keele University; Reino Unido Fil: Ricker, G.. Massachusetts Institute of Technology; Estados Unidos Fil: Vanderspek, R.. Massachusetts Institute of Technology; Estados Unidos Fil: Latham, D.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Seager, S.. Massachusetts Institute of Technology; Estados Unidos Fil: Winn, J. N.. University of Princeton; Estados Unidos Fil: Jenkins, J. M.. National Aeronautics and Space Administration; Estados Unidos Fil: Collins, K. A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Stassun, K. G.. Vanderbilt University; Estados Unidos Fil: Ziegler, C.. University of Toronto; Canadá Fil: Almenara, J. M.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; Francia Fil: Anderson, D. R.. Keele University; Reino Unido. University of Warwick; Reino Unido Fil: Artigau, E.. University of Montreal; Canadá Fil: Bonfils, X.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; Francia Fil: Bouchy, F.. Universidad de Ginebra; Suiza Fil: Briceño, C.. Cerro Tololo Inter American Observatory; Chile Fil: Butler, R. P.. Carnegie Institution for Science; Estados Unidos Fil: Charbonneau, D.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Conti, D. M.. American Association of Variable Star Observers; Estados Unidos Fil: Crane, J.. Observatories of the Carnegie Institution for Science; Estados Unidos Fil: Crossfield, I. J. M.. Massachusetts Institute of Technology; Estados Unidos. University of Kansas; Estados Unidos Fil: Davies, M.. National Aeronautics and Space Administration; Estados Unidos Fil: Delfosse, X.. Universite Grenoble Alpes; Francia. Centre National de la Recherche Scientifique; Francia Fil: Diaz, Rodrigo Fernando. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); Argentina Fil: Doyon, R.. University of Montreal; Canadá
description	We report the detection of a transiting super-Earth-sized planet (R = 1.39 ± 0.09 R⊕ ) in a 1.4-day orbit around L 168-9 (TOI-134), a bright M1V dwarf (V = 11, K = 7.1) located at 25.15 ± 0.02 pc. The host star was observed in the first sector of the Transiting Exoplanet Survey Satellite (TESS) mission. For confirmation and planet mass measurement purposes, this was followed up with ground-based photometry, seeing-limited and high-resolution imaging, and precise radial velocity (PRV) observations using the HARPS and Magellan/PFS spectrographs. By combining the TESS data and PRV observations, we find the mass of L 168-9 b to be 4.60 ± 0.56 M⊕ and thus the bulk density to be 1.74-0.33+0.44 times higher than that of the Earth. The orbital eccentricity is smaller than 0.21 (95% confidence). This planet is a level one candidate for the TESS mission's scientific objective of measuring the masses of 50 small planets, and it is one of the most observationally accessible terrestrial planets for future atmospheric characterization.
publishDate	2020
dc.date.none.fl_str_mv	2020-04
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/11336/151445 Astudillo Defru, Nicola; Cloutier, R.; Wang, S. X.; Teske, J.; Brahm, R.; et al.; A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS; EDP Sciences; Astronomy and Astrophysics; 636; 4-2020; 1-13 0004-6361 1432-0746 CONICET Digital CONICET
url	http://hdl.handle.net/11336/151445
identifier_str_mv	Astudillo Defru, Nicola; Cloutier, R.; Wang, S. X.; Teske, J.; Brahm, R.; et al.; A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS; EDP Sciences; Astronomy and Astrophysics; 636; 4-2020; 1-13 0004-6361 1432-0746 CONICET Digital CONICET
dc.language.none.fl_str_mv	eng
language	eng
dc.relation.none.fl_str_mv	info:eu-repo/semantics/altIdentifier/doi/ info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201937179 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2001.09175
dc.rights.none.fl_str_mv	info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv	openAccess
rights_invalid_str_mv	https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv	application/pdf 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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score	13.070432

A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS

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