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Fig. 1.


Sample realisation from the high-resolution study (see Appendix A) with vBH = 10 km s−1 and bBH = 10−5 pc; (a) with all planets and (b) without terrestrial planets. Both panels show the trajectories of the planets with coloured lines (Mercury ☿, Venus ♀, Earth ⊕, Mars ♂, Jupiter ♃, Saturn ♄, Uranus ♅, Neptune ♆), the Sun (yellow dots), and the BH (black dots). The left panels are plotted in the coordinates fixed to the initial position of the Sun (x0, y0, z0), in which the impactor arrived from the right-hand side, and the right panels show a detailed view of the final system captured by the BH in its co-moving coordinates (xBH, yBH, zBH).

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