Time evolution of inclination for 20   M_Earth planets with individual starting inclinations ranging from i = 1.0° to i = 4.0° in a fully radiative disc. The damping of inclination follows the trend of change of inclination for planets on fixed orbits, see Fig. 1. The black dotted lines indicate our manual fitting with τ_inc = 26.5 for planets with i₀ = 2.0°, 4.0°, 6.0° and i₀ = 8.0°, which seems very good in the beginning/middle phase of the inclination damping. In the i₀ = 8.0° case an additional fit provides for a di/dt ∝ i^-2 fit in the beginning of the evolution.