TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert
- Autores
- Hacker, Alejandro; Díaz, Rodrigo Fernando; Armstrong, David J.; Fernández Fernández, Jorge; Müller, Simon; Delgado Mena, Elisa; Sousa, Sérgio G.; Adibekyan, Vardan; Stassun, Keivan G.; Collins, Karen A.; Yee, Samuel W.; Bayliss, Daniel; Bieryla, Allyson; Bouchy, François; Butler, R. Paul; Crane, Jeffrey D.; Dumusque, Xavier; Hartman, Joel D.; Helled, Ravit; Jenkins, Jon; Keniger, Marcelo Aron F.; Lewis, Hannah; Lillo Box, Jorge; Lund, Michael B.; Nielsen, Louise D.; Watkins, Cristilyn N.; Wheatley, Peter J.; Winn, Joshua N.; Wohler, Bill; Ziegler, Carl
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We report the discovery of two transiting planets detected by the Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V and an F8V star, respectively, with periods of 4.31 and 1.27 d, respectively. We confirm and characterize these two planets with a variety of ground-based and follow-up observations, including photometry, precise radial velocity monitoring and high-resolution imaging. The planetary and orbital parameters were derived from a joint analysis of the radial velocities and photometric data. We found that the two planets have masses of (57 ± 4) M⊕ or (0.18 ± 0.01) MJ, and (68 ± 4) M⊕ or (0.21 ± 0.01) MJ, respectively, and they have radii of (6.8 ± 0.3) R⊕ or (0.61 ± 0.03) RJ and (7.2 ± 0.5) R⊕ or (0.64 ± 0.05) RJ, respectively. These parameters correspond to sub-Saturns within the Neptunian desert, both planets being hot and highly irradiated, with Teq ≈ 745 K and Teq ≈ 1812 K, respectively, assuming a Bond albedo of 0.5. TOI-3071 b has the hottest equilibrium temperature of all known planets with masses between 10 and 300 M⊕ and radii less than 1.5 RJ. By applying gas giant evolution models we found that both planets, especially TOI-3071 b, are very metal-rich. This challenges standard formation models which generally predict lower heavy-element masses for planets with similar characteristics. We studied the evolution of the planets´ atmospheres under photoevaporation and concluded that both are stable against evaporation due to their large masses and likely high metallicities in their gaseous envelopes.
Fil: Hacker, Alejandro. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; Argentina
Fil: Díaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; Argentina
Fil: Armstrong, David J.. University of Warwick; Reino Unido
Fil: Fernández Fernández, Jorge. University of Warwick; Reino Unido
Fil: Müller, Simon. Universitat Zurich; Suiza
Fil: Delgado Mena, Elisa. Universidad de Porto; Portugal
Fil: Sousa, Sérgio G.. Universidad de Porto; Portugal
Fil: Adibekyan, Vardan. Universidad de Porto; Portugal
Fil: Stassun, Keivan G.. Vanderbilt University; Estados Unidos
Fil: Collins, Karen A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Yee, Samuel W.. University of Princeton; Estados Unidos
Fil: Bayliss, Daniel. University of Warwick; Reino Unido
Fil: Bieryla, Allyson. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Bouchy, François. Université de Genève; Suiza
Fil: Butler, R. Paul. Carnegie Institution For Science;
Fil: Crane, Jeffrey D.. Carnegie Institution For Science;
Fil: Dumusque, Xavier. Université de Genève; Suiza
Fil: Hartman, Joel D.. University of Princeton; Estados Unidos
Fil: Helled, Ravit. Universitat Zurich; Suiza
Fil: Jenkins, Jon. National Aeronautics and Space Administration; Estados Unidos
Fil: Keniger, Marcelo Aron F.. University of Warwick; Reino Unido
Fil: Lewis, Hannah. Space Telescope Science Institute; Estados Unidos
Fil: Lillo Box, Jorge. Instituto Nacional de Tecnología Agropecuaria; Argentina. Consejo Superior de Investigaciones Científicas; España
Fil: Lund, Michael B.. National Aeronautics and Space Administration; Estados Unidos. California Institute of Technology; Estados Unidos
Fil: Nielsen, Louise D.. Ludwig Maximilians Universitat; Alemania. European Southern Observatory Chile; Chile
Fil: Watkins, Cristilyn N.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Wheatley, Peter J.. University of Warwick; Reino Unido
Fil: Winn, Joshua N.. University of Princeton; Estados Unidos
Fil: Wohler, Bill. SETI Institute; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos
Fil: Ziegler, Carl. Stephen F. Austin State University; Estados Unidos - Materia
- Astrophysics - Earth and Planetary Astrophysics
- 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:11336/267144
Ver los metadatos del registro completo
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TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desertHacker, AlejandroDíaz, Rodrigo FernandoArmstrong, David J.Fernández Fernández, JorgeMüller, SimonDelgado Mena, ElisaSousa, Sérgio G.Adibekyan, VardanStassun, Keivan G.Collins, Karen A.Yee, Samuel W.Bayliss, DanielBieryla, AllysonBouchy, FrançoisButler, R. PaulCrane, Jeffrey D.Dumusque, XavierHartman, Joel D.Helled, RavitJenkins, JonKeniger, Marcelo Aron F.Lewis, HannahLillo Box, JorgeLund, Michael B.Nielsen, Louise D.Watkins, Cristilyn N.Wheatley, Peter J.Winn, Joshua N.Wohler, BillZiegler, CarlAstrophysics - Earth and Planetary Astrophysicshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We report the discovery of two transiting planets detected by the Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V and an F8V star, respectively, with periods of 4.31 and 1.27 d, respectively. We confirm and characterize these two planets with a variety of ground-based and follow-up observations, including photometry, precise radial velocity monitoring and high-resolution imaging. The planetary and orbital parameters were derived from a joint analysis of the radial velocities and photometric data. We found that the two planets have masses of (57 ± 4) M⊕ or (0.18 ± 0.01) MJ, and (68 ± 4) M⊕ or (0.21 ± 0.01) MJ, respectively, and they have radii of (6.8 ± 0.3) R⊕ or (0.61 ± 0.03) RJ and (7.2 ± 0.5) R⊕ or (0.64 ± 0.05) RJ, respectively. These parameters correspond to sub-Saturns within the Neptunian desert, both planets being hot and highly irradiated, with Teq ≈ 745 K and Teq ≈ 1812 K, respectively, assuming a Bond albedo of 0.5. TOI-3071 b has the hottest equilibrium temperature of all known planets with masses between 10 and 300 M⊕ and radii less than 1.5 RJ. By applying gas giant evolution models we found that both planets, especially TOI-3071 b, are very metal-rich. This challenges standard formation models which generally predict lower heavy-element masses for planets with similar characteristics. We studied the evolution of the planets´ atmospheres under photoevaporation and concluded that both are stable against evaporation due to their large masses and likely high metallicities in their gaseous envelopes.Fil: Hacker, Alejandro. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; ArgentinaFil: Díaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; ArgentinaFil: Armstrong, David J.. University of Warwick; Reino UnidoFil: Fernández Fernández, Jorge. University of Warwick; Reino UnidoFil: Müller, Simon. Universitat Zurich; SuizaFil: Delgado Mena, Elisa. Universidad de Porto; PortugalFil: Sousa, Sérgio G.. Universidad de Porto; PortugalFil: Adibekyan, Vardan. Universidad de Porto; PortugalFil: Stassun, Keivan G.. Vanderbilt University; Estados UnidosFil: Collins, Karen A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Yee, Samuel W.. University of Princeton; Estados UnidosFil: Bayliss, Daniel. University of Warwick; Reino UnidoFil: Bieryla, Allyson. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Bouchy, François. Université de Genève; SuizaFil: Butler, R. Paul. Carnegie Institution For Science;Fil: Crane, Jeffrey D.. Carnegie Institution For Science;Fil: Dumusque, Xavier. Université de Genève; SuizaFil: Hartman, Joel D.. University of Princeton; Estados UnidosFil: Helled, Ravit. Universitat Zurich; SuizaFil: Jenkins, Jon. National Aeronautics and Space Administration; Estados UnidosFil: Keniger, Marcelo Aron F.. University of Warwick; Reino UnidoFil: Lewis, Hannah. Space Telescope Science Institute; Estados UnidosFil: Lillo Box, Jorge. Instituto Nacional de Tecnología Agropecuaria; Argentina. Consejo Superior de Investigaciones Científicas; EspañaFil: Lund, Michael B.. National Aeronautics and Space Administration; Estados Unidos. California Institute of Technology; Estados UnidosFil: Nielsen, Louise D.. Ludwig Maximilians Universitat; Alemania. European Southern Observatory Chile; ChileFil: Watkins, Cristilyn N.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Wheatley, Peter J.. University of Warwick; Reino UnidoFil: Winn, Joshua N.. University of Princeton; Estados UnidosFil: Wohler, Bill. SETI Institute; Estados Unidos. National Aeronautics and Space Administration; Estados UnidosFil: Ziegler, Carl. Stephen F. Austin State University; Estados UnidosWiley Blackwell Publishing, Inc2024-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/267144Hacker, Alejandro; Díaz, Rodrigo Fernando; Armstrong, David J.; Fernández Fernández, Jorge; Müller, Simon; et al.; TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 532; 2; 8-2024; 1612-16340035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/532/2/1612/7690173info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stae1420info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:37:15Zoai:ri.conicet.gov.ar:11336/267144instacron: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:34982025-10-15 14:37:16.183CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert |
| title |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert |
| spellingShingle |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert Hacker, Alejandro Astrophysics - Earth and Planetary Astrophysics |
| title_short |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert |
| title_full |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert |
| title_fullStr |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert |
| title_full_unstemmed |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert |
| title_sort |
TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert |
| dc.creator.none.fl_str_mv |
Hacker, Alejandro Díaz, Rodrigo Fernando Armstrong, David J. Fernández Fernández, Jorge Müller, Simon Delgado Mena, Elisa Sousa, Sérgio G. Adibekyan, Vardan Stassun, Keivan G. Collins, Karen A. Yee, Samuel W. Bayliss, Daniel Bieryla, Allyson Bouchy, François Butler, R. Paul Crane, Jeffrey D. Dumusque, Xavier Hartman, Joel D. Helled, Ravit Jenkins, Jon Keniger, Marcelo Aron F. Lewis, Hannah Lillo Box, Jorge Lund, Michael B. Nielsen, Louise D. Watkins, Cristilyn N. Wheatley, Peter J. Winn, Joshua N. Wohler, Bill Ziegler, Carl |
| author |
Hacker, Alejandro |
| author_facet |
Hacker, Alejandro Díaz, Rodrigo Fernando Armstrong, David J. Fernández Fernández, Jorge Müller, Simon Delgado Mena, Elisa Sousa, Sérgio G. Adibekyan, Vardan Stassun, Keivan G. Collins, Karen A. Yee, Samuel W. Bayliss, Daniel Bieryla, Allyson Bouchy, François Butler, R. Paul Crane, Jeffrey D. Dumusque, Xavier Hartman, Joel D. Helled, Ravit Jenkins, Jon Keniger, Marcelo Aron F. Lewis, Hannah Lillo Box, Jorge Lund, Michael B. Nielsen, Louise D. Watkins, Cristilyn N. Wheatley, Peter J. Winn, Joshua N. Wohler, Bill Ziegler, Carl |
| author_role |
author |
| author2 |
Díaz, Rodrigo Fernando Armstrong, David J. Fernández Fernández, Jorge Müller, Simon Delgado Mena, Elisa Sousa, Sérgio G. Adibekyan, Vardan Stassun, Keivan G. Collins, Karen A. Yee, Samuel W. Bayliss, Daniel Bieryla, Allyson Bouchy, François Butler, R. Paul Crane, Jeffrey D. Dumusque, Xavier Hartman, Joel D. Helled, Ravit Jenkins, Jon Keniger, Marcelo Aron F. Lewis, Hannah Lillo Box, Jorge Lund, Michael B. Nielsen, Louise D. Watkins, Cristilyn N. Wheatley, Peter J. Winn, Joshua N. Wohler, Bill Ziegler, Carl |
| 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 |
Astrophysics - Earth and Planetary Astrophysics |
| topic |
Astrophysics - Earth and Planetary Astrophysics |
| 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 discovery of two transiting planets detected by the Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V and an F8V star, respectively, with periods of 4.31 and 1.27 d, respectively. We confirm and characterize these two planets with a variety of ground-based and follow-up observations, including photometry, precise radial velocity monitoring and high-resolution imaging. The planetary and orbital parameters were derived from a joint analysis of the radial velocities and photometric data. We found that the two planets have masses of (57 ± 4) M⊕ or (0.18 ± 0.01) MJ, and (68 ± 4) M⊕ or (0.21 ± 0.01) MJ, respectively, and they have radii of (6.8 ± 0.3) R⊕ or (0.61 ± 0.03) RJ and (7.2 ± 0.5) R⊕ or (0.64 ± 0.05) RJ, respectively. These parameters correspond to sub-Saturns within the Neptunian desert, both planets being hot and highly irradiated, with Teq ≈ 745 K and Teq ≈ 1812 K, respectively, assuming a Bond albedo of 0.5. TOI-3071 b has the hottest equilibrium temperature of all known planets with masses between 10 and 300 M⊕ and radii less than 1.5 RJ. By applying gas giant evolution models we found that both planets, especially TOI-3071 b, are very metal-rich. This challenges standard formation models which generally predict lower heavy-element masses for planets with similar characteristics. We studied the evolution of the planets´ atmospheres under photoevaporation and concluded that both are stable against evaporation due to their large masses and likely high metallicities in their gaseous envelopes. Fil: Hacker, Alejandro. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; Argentina Fil: Díaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; Argentina Fil: Armstrong, David J.. University of Warwick; Reino Unido Fil: Fernández Fernández, Jorge. University of Warwick; Reino Unido Fil: Müller, Simon. Universitat Zurich; Suiza Fil: Delgado Mena, Elisa. Universidad de Porto; Portugal Fil: Sousa, Sérgio G.. Universidad de Porto; Portugal Fil: Adibekyan, Vardan. Universidad de Porto; Portugal Fil: Stassun, Keivan G.. Vanderbilt University; Estados Unidos Fil: Collins, Karen A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Yee, Samuel W.. University of Princeton; Estados Unidos Fil: Bayliss, Daniel. University of Warwick; Reino Unido Fil: Bieryla, Allyson. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Bouchy, François. Université de Genève; Suiza Fil: Butler, R. Paul. Carnegie Institution For Science; Fil: Crane, Jeffrey D.. Carnegie Institution For Science; Fil: Dumusque, Xavier. Université de Genève; Suiza Fil: Hartman, Joel D.. University of Princeton; Estados Unidos Fil: Helled, Ravit. Universitat Zurich; Suiza Fil: Jenkins, Jon. National Aeronautics and Space Administration; Estados Unidos Fil: Keniger, Marcelo Aron F.. University of Warwick; Reino Unido Fil: Lewis, Hannah. Space Telescope Science Institute; Estados Unidos Fil: Lillo Box, Jorge. Instituto Nacional de Tecnología Agropecuaria; Argentina. Consejo Superior de Investigaciones Científicas; España Fil: Lund, Michael B.. National Aeronautics and Space Administration; Estados Unidos. California Institute of Technology; Estados Unidos Fil: Nielsen, Louise D.. Ludwig Maximilians Universitat; Alemania. European Southern Observatory Chile; Chile Fil: Watkins, Cristilyn N.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Wheatley, Peter J.. University of Warwick; Reino Unido Fil: Winn, Joshua N.. University of Princeton; Estados Unidos Fil: Wohler, Bill. SETI Institute; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos Fil: Ziegler, Carl. Stephen F. Austin State University; Estados Unidos |
| description |
We report the discovery of two transiting planets detected by the Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V and an F8V star, respectively, with periods of 4.31 and 1.27 d, respectively. We confirm and characterize these two planets with a variety of ground-based and follow-up observations, including photometry, precise radial velocity monitoring and high-resolution imaging. The planetary and orbital parameters were derived from a joint analysis of the radial velocities and photometric data. We found that the two planets have masses of (57 ± 4) M⊕ or (0.18 ± 0.01) MJ, and (68 ± 4) M⊕ or (0.21 ± 0.01) MJ, respectively, and they have radii of (6.8 ± 0.3) R⊕ or (0.61 ± 0.03) RJ and (7.2 ± 0.5) R⊕ or (0.64 ± 0.05) RJ, respectively. These parameters correspond to sub-Saturns within the Neptunian desert, both planets being hot and highly irradiated, with Teq ≈ 745 K and Teq ≈ 1812 K, respectively, assuming a Bond albedo of 0.5. TOI-3071 b has the hottest equilibrium temperature of all known planets with masses between 10 and 300 M⊕ and radii less than 1.5 RJ. By applying gas giant evolution models we found that both planets, especially TOI-3071 b, are very metal-rich. This challenges standard formation models which generally predict lower heavy-element masses for planets with similar characteristics. We studied the evolution of the planets´ atmospheres under photoevaporation and concluded that both are stable against evaporation due to their large masses and likely high metallicities in their gaseous envelopes. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024-08 |
| 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 |
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article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/267144 Hacker, Alejandro; Díaz, Rodrigo Fernando; Armstrong, David J.; Fernández Fernández, Jorge; Müller, Simon; et al.; TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 532; 2; 8-2024; 1612-1634 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/267144 |
| identifier_str_mv |
Hacker, Alejandro; Díaz, Rodrigo Fernando; Armstrong, David J.; Fernández Fernández, Jorge; Müller, Simon; et al.; TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 532; 2; 8-2024; 1612-1634 0035-8711 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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openAccess |
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Wiley Blackwell Publishing, Inc |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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