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Aims: We aim to investigate the consequences of a fast massive stellarremnant - a black hole (BH) or a neutron star (NS) - encountering a planetarysystem. Methods: We modelled a close encounter between the actual Solar System(SS) and a $2\,M_\odot$ NS and a $10\,M_\odot$ BH, using a few-body symplecticintegrator. We used a range of impact parameters, orbital phases at the startof the simulation derived from the current SS orbital parameters, encountervelocities, and incidence angles relative to the plane of the SS. Results: Wegive the distribution of possible outcomes, such as when the SS remains bound,when it suffers a partial or complete disruption, and in which cases theintruder is able to capture one or more planets, yielding planetary systemsaround a BH or a NS. We also show examples of the long-term stability of thecaptured planetary systems.

Close encounters with the Death Star: Interactions between collapsed bodies and the Solar System