Surface density and planetesimal eccentricity evolution of the circumstellar disk. We show the gas surface density (blue), planetesimal surface density (black), and the combined dust and pebble surface density (orange) at t = 0.35 Myr, t = 1 Myr, t = 3.5 Myr, and t= 16.8 Myr. The initial corresponding density is shown as the dashed line. The initial mass of the gas disk is given as M(Σ_g) = 34102.64 M_⊕, the initial solid mass in dust and pebbles is given as Μ(Σ_tp) = 450.93 M_⊕, and the initial planetesimal disk mass is given as M(Σ_tp) = 0 M_⊕. The location of an active planet is indicated via dashed vertical lines. The planetesimal eccentricity is given as the dotted line, respectively.