Comparison over the whole mass range, between 0.2 and 1.5 M_⊙, of the rotation period distributions of our solar metallicity models with observations from open clusters of increasing ages (grey crosses, data from Gallet & Bouvier 2013; Bouvier et al. 2014; Douglas et al. 2016, 2017; Agüeros et al. 2018). The red, green, and blue crosses represent the rotation periods of the slow-, median-, and fast-rotating grids, respectively. Masses and ages of cluster members are taken from the literature.