TIC-320687387 B: a long-period eclipsing M-dwarf close to the hydrogen burning limit

Samuel Gill, Solene Ulmer-Moll, Peter J. Wheatley, Daniel Bayliss, Matthew R. Burleigh, Jack S. Acton, Sarah L. Casewell, Christopher A. Watson, Monika Lendl, Hannah L. Worters, Ramotholo R. Sefako, David R. Anderson, Douglas R. Alves, François Bouchy, Edward M. Bryant, Philipp Eigmüller, Edward Gillen, Michael R. Goad, Nolan Grieves, Maximilian N. Günther, Beth A. Henderson, James S. Jenkins, Lokesh Mishra, Maximiliano Moyano, Hugh P. Osborn, Rosanna H. Tilbrook, Stéphane Udry, Jose I. Vines, Richard G. West

Published 2022-01-05Version 1

We are using precise radial velocities from CORALIE together with precision photometry from the Next Generation Transit Survey (NGTS) to follow up stars with single-transit events detected with the Transiting Exoplanet Survey Satellite (TESS). As part of this survey we identified a single transit on the star TIC-320687387, a bright (T=11.6) G-dwarf observed by TESS in Sector 13 and 27. From subsequent monitoring of TIC-320687387 with CORALIE, NGTS, and Lesedi we determined that the companion, TIC-320687387 B,is a very low-mass star with a mass of $96.2 \pm _{2.0}^{1.9} M_J$ and radius of $1.14 \pm _{0.02}^{0.02} R_J$ placing it close to the hydrogen burning limit ($\sim 80 M_J$). TIC-320687387 B has a wide and eccentric orbit, with a period of 29.77381 days and an eccentricity of $0.366 \pm 0.003$. Eclipsing systems such as TIC-320687387 AB allow us to test stellar evolution models for low-mass stars, which in turn are needed to calculate accurate masses and radii for exoplanets orbiting single low-mass stars. The wide orbit of TIC-320687387 B makes it particularly valuable as its evolution can be assumed to be free from perturbations caused by tidal interactions with its G-type host star.