TOI 2093 c in the context of exoplanets with known mass and radius with errors smaller than 12%. Left panel: planetary mass and radius, with theoretical models from Zeng et al. (2016) (see Sect. 4). Right panel: escape velocity against equilibrium temperature (planetary data from the NASA exoplanets database). TOI 2093 b is included assuming i_b ≳ 50°, with the planet radius calculated for a bulk density between 0.5 and 10 g cm⁻³, with errors shown as a red band.