TOI-1268b: The youngest hot Saturn-mass transiting exoplanet
Artikel i vetenskaplig tidskrift, 2022
We report the discovery of TOI-1268b, a transiting Saturn-mass planet from the TESS space mission. With an age of less than 1 Gyr, derived from various age indicators, TOI-1268b is the youngest Saturn-mass planet known to date; it contributes to the small sample of well-characterised young planets. It has an orbital period of P = 8.1577080 ± 0.0000044 days, and transits an early K-dwarf star with a mass of M∗ = 0.96 ± 0.04 M+, a radius of R∗ = 0.92 ± 0.06 R+, an effective temperature of Teff = 5300 ± 100 K, and a metallicity of 0.36 ± 0.06 dex. By combining TESS photometry with high-resolution spectra acquired with the Tull spectrograph at the McDonald Observatory, and the high-resolution spectrographs at the Tautenburg and OndR ejov Observatories, we measured a planetary mass of Mp = 96.4 ± 8.3 Mp and a radius of Rp = 9.1 ± 0.6 Rp. TOI-1268 is an ideal system for studying the role of star-planet tidal interactions for non-inflated Saturn-mass planets. We used system parameters derived in this paper to constrain the planeta's tidal quality factor to the range of 104.5-5.3. When compared with the sample of other non-inflated Saturn-mass planets, TOI-1268b is one of the best candidates for transmission spectroscopy studies.
Techniques: radial velocities
Planets and satellites: gaseous planets
Techniques: spectroscopic
Planetary systems
Planets and satellites: Atmospheres
Techniques: photometric
Författare
J. Šubjak
Czech Academy of Sciences
European Southern Observatory (ESO)
Univerzita Karlova
M. Endl
The University of Texas at Austin
Priyanka Chaturvedi
Thüringer Landessternwarte Tautenburg
R. Karjalainen
Czech Academy of Sciences
William D. Cochran
The University of Texas at Austin
M. Esposito
Thüringer Landessternwarte Tautenburg
D. Gandolfi
Universita degli Studi di Torino
K. W.F. Lam
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
Technische Universität Berlin
Keivan G. Stassun
Fisk University
Vanderbilt University
Jirí Žák
European Southern Observatory (ESO)
N. Lodieu
Instituto de Astrofísica de Canarias
Universidad de la Laguna
Henri M. J. Boffin
European Southern Observatory (ESO)
P. MacQueen
The University of Texas at Austin
A. Hatzes
Thüringer Landessternwarte Tautenburg
E. W. Guenther
Thüringer Landessternwarte Tautenburg
Iskra Georgieva
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
S. Grziwa
Universität zu Köln
H. Schmerling
Universität zu Köln
Marek Skarka
Czech Academy of Sciences
M. Blažek
Czech Academy of Sciences
Masarykova Univerzita
M. Karjalainen
Czech Academy of Sciences
Magdalena Špoková
Czech Academy of Sciences
Masarykova Univerzita
H. Isaacson
University of California
A. W. Howard
California Institute of Technology (Caltech)
Christopher J. Burke
Massachusetts Institute of Technology (MIT)
Vincent Van Eylen
University College London (UCL)
B. Falk
Space Telescope Science Institute (STScI)
Malcolm Fridlund
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Universiteit Leiden
E. Goffo
Universita degli Studi di Torino
Thüringer Landessternwarte Tautenburg
Jon M. Jenkins
NASA Ames Research Center
Judith Korth
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Jack J. Lissauer
NASA Ames Research Center
J.H. Livingston
National Astronomical Observatory of Japan
University of Tokyo
National Institutes of Natural Sciences
R. Luque
Instituto de Astrofisica de Andalucía (IAA)
Alexandra Muresan
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
H. P. Osborn
Massachusetts Institute of Technology (MIT)
Universität Bern
Enric Palle
Universidad de la Laguna
Instituto de Astrofísica de Canarias
Carina Persson
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
S. Redfield
Wesleyan University
George R. Ricker
Massachusetts Institute of Technology (MIT)
S. Seager
Massachusetts Institute of Technology (MIT)
L. M. Serrano
Universita degli Studi di Torino
Alexis M. S. Smith
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
Petr Kabath
Czech Academy of Sciences
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 662 A107Ämneskategorier
Subatomär fysik
Analytisk kemi
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202142883