
Judith Korth
Postdoc

TOI-220 b : A warm sub-Neptune discovered by TESS
Author
Summary, in English
In this paper, we report the discovery of TOI-220 b, a new sub-Neptune detected by the Transiting Exoplanet Survey Satellite (TESS) and confirmed by radial velocity follow-up observations with the HARPS spectrograph. Based on the combined analysis of TESS transit photometry and high precision radial velocity measurements, we estimate a planetary mass of 13.8 ± 1.0 M⊕ and radius of 3.03 ± 0.15 R⊕, implying a bulk density of 2.73 ± 0.47 g cm-3. TOI-220 b orbits a relative bright (V= 10.4) and old (10.1 ± 1.4 Gyr) K dwarf star with a period of ∼10.69 d. Thus, TOI-220 b is a new warm sub-Neptune with very precise mass and radius determinations. A Bayesian analysis of the TOI-220 b internal structure indicates that due to the strong irradiation it receives, the low density of this planet could be explained with a steam atmosphere in radiative-convective equilibrium and a supercritical water layer on top of a differentiated interior made of a silicate mantle and a small iron core.
Publishing year
2021-08-01
Language
English
Pages
3361-3379
Publication/Series
Monthly Notices of the Royal Astronomical Society
Volume
505
Issue
3
Document type
Journal article
Publisher
Oxford University Press
Keywords
- planets and satellites: fundamental parameters
- planets and satellites: individual: TYC 8897-01263-1
- stars: fundamental parameters
- techniques: photometric
- techniques: radial velocities
Status
Published
ISBN/ISSN/Other
- ISSN: 0035-8711