Nucleation rates, J_*,i [cm⁻³ s⁻¹] (dashed lines), in the extended, low-pressure extrapolated substellar, antistellar, and equatorial morning and evening terminator (T_gas, p_gas)-profiles (solid dark grey lines) for the G star planet atmosphere (T_eff,P = 1600 K, log(ɡ) = 3 [cgs]). The nucleation rates for TiO₂ (dark blue), SiO (brown), KCl (magenta), NaCl (cyan) and the thermal stability curves (supersaturation ratio S = 1 for solar element abundances; dotted lines) for their respective solid condensates are shown. The S_i = 1 curves do not represent our full kinetic model approach and are provided here for the purpose of visualisation only.