The mass-radius relation of exoplanets, revisited

Determining the mass-radius (M-R) relation of exoplanets is important for exoplanet characterization. Here we present a re-analysis of the M-R relations and their transitions using exoplanetary data from the PlanetS catalog which only includes planets with reliable mass and radius determinations. We find that "small planets" correspond to planets with masses of up to ∼4.4 M_⊕ (within 17 with masses between ∼4.4 and 127 M_⊕ (within 5 "intermediate-mass" planets, where R ∝ M^0.67. Massive planets, or gas giant planets, are found to have masses beyond 127 M_⊕ with an M-R relation of R ∝ M^-0.06. By analyzing the radius-density relation we also find that the transition between "small" to "intermediate-size" planets occurs at a planetary radius of ∼1.6 R_⊕ (within 3 ideal fit for the currently-measured planetary population.