Mass-loss rate as a function of stellar age for comparison of rotationally induced mass loss. The red solid lines represent models with default MESA settings of rotationally induced Ṁ (see Eq. (1)), with an initial mass of 40 M_⊙ and rotation rates of 100 km s⁻¹ and 300 km s⁻¹. All other processes have been set to default values to avoid conflict in our analysis. The dashed blue lines show the corresponding models with ξ = 0, for the same mass and rotation rates respectively.