Radiative force of the total crater averaged over a rotational period (8 h by default) obtained from the analytical method (solid lines) and the numerical method (dashed lines), as a function of the crater colatitude α for K = 2.65 Wm⁻¹ K⁻¹ (left panel) and K = 0.1 Wm⁻¹ K⁻¹ (right panel). The x, y, and 𝓏 components of the radiative force are shown in blue, red, and green, respectively. The distance of the crater here is 1 au from the Sun.