Evolution of the planetary mass estimated by considering different rotational histories for η = 0.1 and R_XUV∕R_pl = 1. The yellow shaded area shows the evolution for Ω_in = 1 Ω_⊙, the cyan shaded area for Ω_in = 3.2 Ω_⊙, and the green shaded area for Ω_in = 5 Ω_⊙. The black hatched area shows the evolution for Ω_in = Ω_⊙, which is the range of initial masses compatible with an initial Ganymede-like composition.