Evolution of computed surface abundance patterns in XEVOL models T150KD1K-3 (first nine profiles) and T65KD10--4 (last profile), for star HD 318101, with M_* = 4.7 ﹩\;{M}_{\odot }﹩. The top legend indicates the age, effective temperature, and level of turbulence of each model. Observations from R. Monier (2015, private communication, black circles) and this paper (red triangles) are shown for comparison. Scandium, measured but not included in the simulations, is shown as a gray triangle. Lines for ages >99 Myr correspond to the end of the main sequence and the rapid wiping out of anomalies. Elements for which there are both measurements and modeled values appear in red at the top of the plot. Abundances are relative to the Sun.