Graphic overview of the disks and final simulated planets in each formation scenario. Left: embryos of different masses (the biggest circles), and pebbles (the smallest circles) or planetesimals (medium circles) located either inside (brown) or outside (blue) the H₂O snowline in a gas disk with low viscosity (curved black arrows) or high viscosity (spiral black arrows). Right: planets with masses <0.5 M_⊙ (violet circles), 0.5 < M/M_⊕ < 1 (blue circles), 1 < M/M_⊕ < 2 (red circles), 2 < M/M_⊕ < 5 (green circles), 5 < M/M_⊕ < 10 (yellow circles) and 10 < M/M_⊕ < 20 (black circles). The percentage of simulations in which planets in each mass range were formed is given below the circles.