LHS 475 b: A Venus-sized Planet Orbiting a Nearby M Dwarf

Based on photometric observations by TESS, we present the discovery of a Venus-sized planet transiting LHS 475, an M3 dwarf located 12.5 pc from the Sun. The mass of the star is \(0.274 \pm 0.015~\rm{M_{Sun}}\). The planet, originally reported as TOI 910.01, has an orbital period of \(2.0291025 \pm 0.0000020\) days and an estimated radius of \(0.955 \pm 0.053~\rm{R_{Earth}}\). We confirm the validity and source of the transit signal with MEarth ground-based follow-up photometry of five individual transits. We present radial velocity data from CHIRON that rule out massive companions. In accordance with the observed mass-radius distribution of exoplanets as well as planet formation theory, we expect this Venus-sized companion to be terrestrial, with an estimated RV semi-amplitude close to 1.0 m/s. LHS 475 b is likely too hot to be habitable but is a suitable candidate for emission and transmission spectroscopy.