Same as in Fig. 13, but now using the second of our convergence criteria. In this case we monitored distance of the (1270) Datura clones from those of family members in Cartesian space and in the same time evaluated their relative velocity. When both quantities became smaller than chosen threshold values, ideally the estimated radius of the Hill sphere of Datura-family parent body and its escape velocity, we considered the configuration converging. The light gray histograms show normalized appearance of converging cases in 10 kyr bins for distance limit of 5000 km and the velocity limit of 10 m s^-1. The dark gray cases have instead 2500 km and 5 m s^-1 limits.