
Judith Korth
Postdoc

TOI-2285b : A 1.7 Earth-radius planet near the habitable zone around a nearby M dwarf
Author
Summary, in English
We report the discovery of TOI-2285b, a sub-Neptune-sized planet transiting a nearby (42 pc) M dwarf with a period of 27.3 d. We identified the transit signal from the Transiting Exoplanet Survey Satellite photometric data, which we confirmed with ground-based photometric observations using the multiband imagers MuSCAT2 and MuSCAT3. Combining these data with other follow-up observations including high-resolution spectroscopy with the Tillinghast Reflector Echelle Spectrograph, high-resolution imaging with the SPeckle Polarimeter, and radial velocity (RV) measurements with the InfraRed Doppler instrument, we find that the planet has a radius of 1.74 ± 0.08, R⊕, a mass of < 19.5 M⊕ (95% c.l.), and an insolation flux of 1.54 ± 0.14 times that of the Earth. Although the planet resides just outside the habitable zone for a rocky planet, if the planet harbors an H2O layer under a hydrogen-rich atmosphere, then liquid water could exist on the surface of the H2O layer depending on the planetary mass and water mass fraction. The bright host star in the near-infrared (Ks = 9.0) makes this planet an excellent target for further RV and atmospheric observations to improve our understanding of the composition, formation, and habitability of sub-Neptune-sized planets.
Publishing year
2022-02-01
Language
English
Pages
1-8
Publication/Series
Publications of the Astronomical Society of Japan
Volume
74
Issue
1
Document type
Journal article
Publisher
Oxford University Press
Keywords
- planets and satellites: detection
- planets and satellites: individual (TOI-2285b)
- planets and satellites: interiors
- techniques: photometric
- techniques: radial velocities
Status
Published
ISBN/ISSN/Other
- ISSN: 0004-6264