Mass-distance diagrams of specific systems with 100 embryos initially (panels a–w), which are taken from the nominal population predicted for a 1 M_⊙ star (NG76). Symbols are as follows: red points show gas-rich planets where M_env ∕M_core > 1. Blue symbols are planets that have accreted some volatile material (ices) outside of the ice line(s). Green symbols are planets that have only accreted refractory solids. Open green and blue circles have 0.1_env ∕M_core ≤ 1 while filled green points and blue crosses have M_env∕M_core ≤ 0.1. For all these bodies, the grey horizontal bars go from a − e to a + e. The top leftpanel with black crosses shows the solar system. Bodies lost because of collisions or ejections are shown in light grey. Planets accreted by the central star are show in the very left of each panel, the ejected ones on the very right and planets that collided with another (more massive) planet are shown at their last position on the diagram. The dotted vertical line in each system shows the location of the ice line. The number after each panel name is the metallicity [M/H] of the system expressed in dex, while the value on the top right is the initial mass of the planetesimals disc.