Fraction of the planetesimal disk mass (M_D(Σ_P)) and combined dust and pebble disk mass (M_D(Σ_tp)) over the gas disk mass (M_D(Σ_g)) within 1 au, 2.5 au, and 5 au over time in percent. The grey dotted line indicates the global initial dust to gas ratio d_g = 1.34%. 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. The total mass in the planetesimal disk after the dispersal of the gas disk is given as 67.59 M_⊕. The final planetesimal disk mass within 5 au is given as 10.5 M_⊕, within 2.5 au as 0.349 M_⊕, and within 1 au as 2.35 × 10⁻³ M_⊕.