Same as Fig. 5, but now, a planet is included in the disk. The viscosity is kept constant, but u_frag is varied. Simulations where the planet was placed at three different locations are shown, relative to the Fe₃O₄, H₂O and CO₂ ice lines. Each column represents a different planet placement, with it being placed further out going from the left-most to the right-most column. The top row depicts disks with u_frag = 1 m s⁻¹ and the bottom row those with u_frag = 10 m s⁻¹.