The ejection velocities of interstellar objects signpost their progenitor system architectures
We investigated how the initial architectures of planetary systems impact the production and kinematics of interstellar objects. Using N-body simulations of 2,461 planetary configurations, we tracked how dynamical instabilities eject planetesimals into interstellar space. We find that typical ejections are relatively slow, causing unbound planetesimals to form compact tidal streams — meaning future surveys like LSST are well-positioned to detect multiple ISOs from the same native system.


