Outcomes of the BH scenario for v_BH = 10 km s⁻¹. For each impact parameter (coded by colours and symbols) and incidence angle (columns), we plotted the final distribution of semi-major axes, eccentricities, and inclinations of planets that were either retained by the Sun or captured by the BH (top six rows, for each planet from Mercury ☿ to Neptune ♆). Bottom two rows: fraction of retained and captured planets. Each variation in the initial parameters was averaged over nine pre-evolved states of the SS, see Sect. 2. Detailed plots for all v_BH and θ_BH are in Figs. B.1–B.8.