TOI-257b (HD 19916b): A Warm sub-Saturn on a Moderately Eccentric Orbit Around an Evolved F-type Star
Brett C. Addison,Duncan J. Wright,Belinda A. Nicholson,Bryson Cale,Teo Mocnik,Daniel Huber,Peter Plavchan,Robert A. Wittenmyer,Andrew Vanderburg,William J. Chaplin,Ashley Chontos,Jake T. Clark,Jason D. Eastman,Carl Ziegler,Rafael Brahm,B. D. Carter,Mathieu Clerte,Néstor Espinoza,Jonathan Horner,J. S. Bentley,Stephen R. Kane,John F. Kielkopf,Emilie Laychock,Matthew W. Mengel,Jack Okumura,Keivan G. Stassun,Timothy R. Bedding,Brendan P. Bowler,Andrius Burnelis,Michaela Collins,Ian J. M. Crossfield,Allen B. Davis,Dag Evensberget,Alexis Heitzmann,Steve B. Howell,Nicholas M. Law,Andrew W. Mann,Stephen C. Marsden,J. O'Connor,Avi Shporer,Catherine Stevens,C. G. Tinney,Christopher Tylor,Songhu Wang,Hui Zhang,Thomas Henning,Diana Kossakowski,George R. Ricker,Paula Sarkis,Roland Vanderspek,David W. Latham,Sara Seager,Joshua N. Winn,Jon M. Jenkins,Ismael Mireles,Pamela Rowden,Joshua Pepper,Tansu Daylan,Joshua E. Schlieder,Karen A. Collins,Kevin I. Collins,Thiam-Guan Tan,Warrick H. Ball,Sarbani Basu,Derek Buzasi,Tiago L. Campante,Enrico Corsaro,L. González-Cuesta,Guy R. Davies,Rafael ~A. ~Garcí a,Zhao Guo,Rasmus Handberg,Saskia Hekker,Daniel R. Hey,Thomas Kallinger,Steven D. Kawaler,Cenk Kayhan,James S. Kuszlewicz,Mikkel N. Lund,Alexander Lyttle,Savita Mathur,Andrea Miglio,Benoit Mosser,Martin Bo Nielsen,Aldo Serenelli,Victor Silva Aguirre,Nathalie Themessl +86 more
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In this paper, the authors reported the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS) and confirmed to be of planetary origin based on radial-velocity observations with the Minerva-Australis telescope array.Abstract:
We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS and confirmed to be of planetary origin based on radial-velocity observations with the Minerva-Australis telescope array. An analysis of the TESS photometry, the Minerva-Australis, FEROS, and HARPS radial velocities, and the asteroseismic data of the stellar oscillations reveals that TOI-257b has a mass of $M_P=0.134^{+0.023}_{-0.022}$$\rm{M_J}$ ($42.6^{+7.3}_{-7.0}$$\rm{M_{\oplus}}$), a radius of $R_P=0.626^{+0.013}_{-0.012}$$\rm{R_J}$ ($7.02^{+0.15}_{-0.13}$$\rm{R_{\oplus}}$), and an orbit with eccentricity $0.242^{+0.040}_{-0.065}$ and period $18.38827\pm0.00072$$\rm{days}$. TOI-257b orbits a bright ($\mathrm{V}=7.570$mag) somewhat evolved late F-type star with $M_*=1.390\pm0.046$$\rm{M_{\odot}}$, $R_*=1.888\pm0.033$$\rm{R_{\odot}}$, $T_{\rm eff}=6075\pm90$$\rm{K}$, and $v\sin{i}=11.3\pm0.5$km/s. Additionally, we statistically validate a second non-transiting sub-Saturn mass planet on a $\sim71$day orbit using the radial velocity data. This system joins the ranks of a small number of exoplanet host stars that have been characterized with asteroseismology. Warm sub-Saturns are rare in the known sample of exoplanets, and thus the discovery of TOI-257b is important in the context of future work studying the formation and migration history of similar planetary systems.read more
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