Geometric albedos and equilibrium temperatures for the five Kepler planets, colored by the inhomogeneous model weight. Model comparisons with weights approaching unity confidently prefer the inhomogeneous model over the homogenous model (see Sect. 3.2), so darker points are more likely inhomogeneous reflectors. The marker shape corresponds to the preferred scattering phase function: squares are Cornette–Shanks single scattering plus isotropic multiple scattering, and circles are isotropic single plus isotropic multiple scattering. Results are also enumerated in Table 2.