Left panel: Rotational period vs effective temperature for stars in clusters of different ages from Curtis et al. (2020). The location of Gl 410 is indicated in solid lines (error on T_eff is given in light red). Right panel: Gaia DR3 color-magnitude diagram of young stars with calibrated ages (dots) and empirical age sequences from young associations (Gagné et al. 2021). The position of Gl 410 is indicated with a red dot. Gl 410 is located between the 400 and 580 Myr sequences.