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spelling todo:paper_00046361_v604_n_p_Osborn2023-10-03T14:01:12Z K2-110 b: A massive mini-Neptune exoplanet Osborn, H.P. Santerne, A. Barros, S.C.C. Santos, N.C. Dumusque, X. Malavolta, L. Armstrong, D.J. Hojjatpanah, S. Demangeon, O. Adibekyan, V. Almenara, J.-M. Barrado, D. Bayliss, D. Boisse, I. Bouchy, F. Brown, D.J.A. Cameron, A.C. Charbonneau, D. Deleuil, M. Delgado Mena, E. DIáz, R.F. Hébrard, G. Kirk, J. King, G.W. Lam, K.W.F. Latham, D. Lillo-Box, J. Louden, T.M. Lovis, C. Marmier, M. McCormac, J. Molinari, E. Pepe, F. Pollacco, D. Sousa, S.G. Udry, S. Walker, S.R. Planets and satellites: Detection Earth (planet) Earth atmosphere Extrasolar planets Photometry Planets Satellites Stars Dwarf stars Exoplanet Follow up H2 atmosphere High-precision Hydrogen atmosphere Joint analysis Planets and satellites: detections Orbits We report the discovery of the exoplanet K2-110 b (previously EPIC212521166b) from K2 photometry orbiting in a 13.8637d period around an old, metal-poor K3 dwarf star. With a V-band magnitude of 11.9, K2-110 is particularly amenable to RV follow-up. A joint analysis of K2 photometry and high-precision RVs from 28 HARPS and HARPS-N spectra reveal it to have a radius of 2.6 ± 0.1R ⊕ and a mass of 16.7 ± 3.2M ⊕ , hence a density of 5.2 ± 1.2 g cm -3 , making it one of the most massive planets yet to be found with a sub-Neptune radius. When accounting for compression, the resulting Earth-like density is best fitted by a 0.2M ⊕ hydrogen atmosphere over an 16.5M ⊕ Earth-like interior, although the planet could also have significant water content. At 0.1 AU, even taking into account the old stellar age of 8 ± 3 Gyr, the planet is unlikely to have been significantly affected by EUV evaporation. However the planet likelydisc-migrated to its current position making the lack of a thick H 2 atmosphere puzzling. This analysis has made K2-110 b one of the best-characterised mini-Neptunes with density constrained to less than 30%. © 2017 ESO. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00046361_v604_n_p_Osborn
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Planets and satellites: Detection
Earth (planet)
Earth atmosphere
Extrasolar planets
Photometry
Planets
Satellites
Stars
Dwarf stars
Exoplanet
Follow up
H2 atmosphere
High-precision
Hydrogen atmosphere
Joint analysis
Planets and satellites: detections
Orbits
spellingShingle Planets and satellites: Detection
Earth (planet)
Earth atmosphere
Extrasolar planets
Photometry
Planets
Satellites
Stars
Dwarf stars
Exoplanet
Follow up
H2 atmosphere
High-precision
Hydrogen atmosphere
Joint analysis
Planets and satellites: detections
Orbits
Osborn, H.P.
Santerne, A.
Barros, S.C.C.
Santos, N.C.
Dumusque, X.
Malavolta, L.
Armstrong, D.J.
Hojjatpanah, S.
Demangeon, O.
Adibekyan, V.
Almenara, J.-M.
Barrado, D.
Bayliss, D.
Boisse, I.
Bouchy, F.
Brown, D.J.A.
Cameron, A.C.
Charbonneau, D.
Deleuil, M.
Delgado Mena, E.
DIáz, R.F.
Hébrard, G.
Kirk, J.
King, G.W.
Lam, K.W.F.
Latham, D.
Lillo-Box, J.
Louden, T.M.
Lovis, C.
Marmier, M.
McCormac, J.
Molinari, E.
Pepe, F.
Pollacco, D.
Sousa, S.G.
Udry, S.
Walker, S.R.
K2-110 b: A massive mini-Neptune exoplanet
topic_facet Planets and satellites: Detection
Earth (planet)
Earth atmosphere
Extrasolar planets
Photometry
Planets
Satellites
Stars
Dwarf stars
Exoplanet
Follow up
H2 atmosphere
High-precision
Hydrogen atmosphere
Joint analysis
Planets and satellites: detections
Orbits
description We report the discovery of the exoplanet K2-110 b (previously EPIC212521166b) from K2 photometry orbiting in a 13.8637d period around an old, metal-poor K3 dwarf star. With a V-band magnitude of 11.9, K2-110 is particularly amenable to RV follow-up. A joint analysis of K2 photometry and high-precision RVs from 28 HARPS and HARPS-N spectra reveal it to have a radius of 2.6 ± 0.1R ⊕ and a mass of 16.7 ± 3.2M ⊕ , hence a density of 5.2 ± 1.2 g cm -3 , making it one of the most massive planets yet to be found with a sub-Neptune radius. When accounting for compression, the resulting Earth-like density is best fitted by a 0.2M ⊕ hydrogen atmosphere over an 16.5M ⊕ Earth-like interior, although the planet could also have significant water content. At 0.1 AU, even taking into account the old stellar age of 8 ± 3 Gyr, the planet is unlikely to have been significantly affected by EUV evaporation. However the planet likelydisc-migrated to its current position making the lack of a thick H 2 atmosphere puzzling. This analysis has made K2-110 b one of the best-characterised mini-Neptunes with density constrained to less than 30%. © 2017 ESO.
format JOUR
author Osborn, H.P.
Santerne, A.
Barros, S.C.C.
Santos, N.C.
Dumusque, X.
Malavolta, L.
Armstrong, D.J.
Hojjatpanah, S.
Demangeon, O.
Adibekyan, V.
Almenara, J.-M.
Barrado, D.
Bayliss, D.
Boisse, I.
Bouchy, F.
Brown, D.J.A.
Cameron, A.C.
Charbonneau, D.
Deleuil, M.
Delgado Mena, E.
DIáz, R.F.
Hébrard, G.
Kirk, J.
King, G.W.
Lam, K.W.F.
Latham, D.
Lillo-Box, J.
Louden, T.M.
Lovis, C.
Marmier, M.
McCormac, J.
Molinari, E.
Pepe, F.
Pollacco, D.
Sousa, S.G.
Udry, S.
Walker, S.R.
author_facet Osborn, H.P.
Santerne, A.
Barros, S.C.C.
Santos, N.C.
Dumusque, X.
Malavolta, L.
Armstrong, D.J.
Hojjatpanah, S.
Demangeon, O.
Adibekyan, V.
Almenara, J.-M.
Barrado, D.
Bayliss, D.
Boisse, I.
Bouchy, F.
Brown, D.J.A.
Cameron, A.C.
Charbonneau, D.
Deleuil, M.
Delgado Mena, E.
DIáz, R.F.
Hébrard, G.
Kirk, J.
King, G.W.
Lam, K.W.F.
Latham, D.
Lillo-Box, J.
Louden, T.M.
Lovis, C.
Marmier, M.
McCormac, J.
Molinari, E.
Pepe, F.
Pollacco, D.
Sousa, S.G.
Udry, S.
Walker, S.R.
author_sort Osborn, H.P.
title K2-110 b: A massive mini-Neptune exoplanet
title_short K2-110 b: A massive mini-Neptune exoplanet
title_full K2-110 b: A massive mini-Neptune exoplanet
title_fullStr K2-110 b: A massive mini-Neptune exoplanet
title_full_unstemmed K2-110 b: A massive mini-Neptune exoplanet
title_sort k2-110 b: a massive mini-neptune exoplanet
url http://hdl.handle.net/20.500.12110/paper_00046361_v604_n_p_Osborn
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