TOI-836: A super-Earth and mini-Neptune transiting a nearby K-dwarf
Abstract
We present the discovery of two exoplanets transiting TOI-836 (TIC 440887364) using data from TESS Sector 11 and Sector 38. TOI-836 is a bright (T = 8.5 mag), high proper motion (~200 mas yr-1), low metallicity ([Fe/H]≈-0.28) K-dwarf with a mass of 0.68 ± 0.05 M⊙ and a radius of 0.67 ± 0.01 R⊙. We obtain photometric follow-up observations with a variety of facilities, and we use these data sets to determine that the inner planet, TOI-836 b, is a 1.70 ± 0.07 R⊕ super-Earth in a 3.82-d orbit, placing it directly within the so-called 'radius valley'. The outer planet, TOI-836 c, is a 2.59 ± 0.09 R⊕ mini-Neptune in an 8.60-d orbit. Radial velocity measurements reveal that TOI-836 b has a mass of 4.5 ± 0.9 M⊕, while TOI-836 c has a mass of 9.6 ± 2.6 M⊕. Photometric observations show Transit Timing Variations (TTVs) on the order of 20 min for TOI-836 c, although there are no detectable TTVs for TOI-836 b. The TTVs of planet TOI-836 c may be caused by an undetected exterior planet.
- Publication:
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Monthly Notices of the Royal Astronomical Society
- Pub Date:
- April 2023
- DOI:
- arXiv:
- arXiv:2208.07328
- Bibcode:
- 2023MNRAS.520.3649H
- Keywords:
-
- techniques: photometric;
- techniques: radial velocities;
- planets and satellites: detection;
- stars: individual: TOI-836 (TIC 440887364;
- GAIA EDR3 6230733559097425152);
- Astrophysics - Earth and Planetary Astrophysics
- E-Print:
- doi:10.1093/mnras/stad306