Comparison of Jupiter’s bulk metallic content between different formation locations, assuming the initial planetesimalsurface density (Σ₁) corresponds to 2, 5 and 10 MMSN at their given location. Σ₁ for each run is shown in Table D.2. The initial core mass for all cases is the same as the one assumed in the nominal setup: 4 ≤ M_core,1 ≤ 17 M_⊕. The lighter colours remark the cases where the meteoritic constraints of K17 are met. The accretion of solids in the detached phase is given by SI08.