Solid mass evolution during the lifetime of the gas disk. We show the total pebble and dust disk mass (M_D(Σ_tp)), the total planetesimal disk mass (M_D(Σ_P)), the mass in active planetary cores (M_c(active)), the mass of all formed planetary cores (M_C(formed)), and and the mass of planetary cores that have been accreted by the host star (M_C(accreted)). The dashed vertical lines are drawn at 0.35 Myr, 1 Myr, and 3.5 Myr and show the moments at which most currently active planets are accreted by the host star or were subject to mergers.