Abstract
We present the discovery and validation of a super-Earth planet orbiting the M dwarf star TOI-1846 (TIC 198385543). The host star () is located 47 pc away and has a radius of, a mass of and an effective temperature of K. Our analyses are based on joint modelling of Transiting Exoplanet Survey Satellite (TESS) photometry and ground-based multicolour photometric data. We also use high-resolution imaging and archival images, as well as statistical validation techniques to support the planetary system nature. We find that TOI-1846 b is a super-Earth sized planet with radius of and a predicted mass of (from the Chen & Kipping relation) on a 3.9 d orbit, with an equilibrium temperature of (assuming a null Bond Albedo) and an incident flux of. Based on the two radial velocity (RV) measurements obtained with the Tillinghast Reflector Echelle Spectrograph and high-resolution imaging, a non-planetary transiting companion is excluded. With a radius of 1.8, TOI-1846 b is within the sparsely populated radius range around 2 known as the radius gap (or radius valley). This discovery can contribute to refining the precise location of the radius valley for small planets orbiting bright M dwarfs, thereby enhancing our understanding of planetary formation and evolution processes.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 3249-3268 |
| Number of pages | 20 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 541 |
| Issue number | 4 |
| DOIs | |
| State | Published - Aug 1 2025 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- planetary systems
- planets and satellites
- stars: individual: (TIC 198385543
- TOI 1846)