Mass-radius diagramofall known transiting exoplanets taken from TepCat(Southworth 2011). Theupperlimits forthe masses of TOI-2095b and TOI-2095c derived from RV measurements (M_b < 4.1 M_⊕ and M_c < 7.4 M_⊕ respectively) are delimited by the black arrows. The predicted masses and uncertainties for TOI-2095b and TOI-2095c computed with the mass-radius relations of Chen & Kipping (2017, left) and Kanodia et al. (2019, right) are marked by the yellow and light blue star respectively. We show planets with P < 30 days and with mass determinations with an uncertainty better than 30%. Planets around stars with T_eff ≤ 4000 K and T_eff > 4000 K are marked by orange circles and blue triangles, respectively. The lines represent the composition models of Zeng et al. (2016, 2019) for pure iron cores (100% Fe, brown solid line), Earth-like rocky compositions (32.5% Fe plus 67.5% MgSiO₃, dash green line), and a water world (0.1% H₂ envelope plus 49.95% Earth-like rocky core plus 49.95% H₂O, dash-dotted blue line).