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Circumbinary planets whose orbits become unstable may be ejected, accreted,or even captured by one of the stars. We quantify the relative rates of thesechannels, for a binary of secondary star's mass fraction 0.1 with an orbit of1AU. The most common outcome is ejection, which happens ~80% of the time. Ifbinary systems form circumbinary planets readily and sloppily, this process mayfill the Milky Way with free-floating planets. A significant fraction of thetime, ~20%, the unstable planet strikes the primary or secondary. We trackedwhether a Jupiter-like planet would undergo tidal stripping events during closepassages, and find that these events are not strong enough to change thetrajectory of the planet, though this may be observable from a changedstructured for free-floating planets that are produced by this process.

On the Fate of Unstable Circumbinary Planets: Tatooine's Close Encounters with a Death Star