An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685

Abstract

Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated planets, can be studied by characterizing the ultra-short-period planet population, which the TESS mission is particularly well suited to discover. Here, we report on the follow-up of a transit signal detected in the TESS sector 19 photometric time series of the M3.0 V star TOI-1685 (2MASS J04342248+4302148). We confirm the planetary nature of the transit signal, which has a period of P b = 0.6691403 −0.0000021 +0.0000023 d, using precise radial velocity measurements taken with the CARMENES spectrograph. From the joint photometry and radial velocity analysis, we estimate the following parameters for TOI-1685 b: a mass of M b = 3.78 −0.63 +0.63 M ⊕ , a radius of R b = 1.70 −0.07 +0.07 R ⊕ , which together result in a bulk density of ρ b = 4.21 −0.82 +0.95 g cm −3 , and an equilibrium temperature of T eq = 1069 −16 +16 K. TOI-1685 b is the least dense ultra-short-period planet around an M dwarf known to date. TOI-1685 b is also one of the hottest transiting super-Earth planets with accurate dynamical mass measurements, which makes it a particularly attractive target for thermal emission spectroscopy. Additionally, we report with moderate evidence an additional non-transiting planet candidate in the system, TOI-1685 [c], which has an orbital period of P c = 9.02 −0.12 +0.10 d.