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<SUP>-1</SUP>), low metallicity ([Fe/H]≈-0.28) K-dwarf with a mass of 0.68 ± 0.05 M<SUB>⊙</SUB> and a radius of 0.67 ± 0.01 R<SUB>⊙</SUB>. 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<SUB>⊕</SUB> 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<SUB>⊕</SUB> 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<SUB>⊕</SUB>, while TOI-836 c has a mass of 9.6 ± 2.6 M<SUB>⊕</SUB>. 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.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
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Bayliss, Daniel; University of Warwick, Department of Physics, University of Warwick, UK
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Collins, Karen A.; Harvard Smithsonian Center for Astrophysics
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