Capture of interstellar objects: a source of long-period comets

Abstract

We simulate the passage through the Sun-Jupiter system of interstellar objects (ISOs) similar to 1I/`Oumuamua or 2I/Borisov. Capture of such objects is rare and overwhelmingly from low incoming speeds onto orbits akin to those of known long-period comets. This suggests that some of these comets could be of extra-solar origin, in particular inactive ones. Assuming ISOs follow the local stellar velocity distribution, we infer a volume capture rate of $0.051{\mathrm{au}}^3{\mathrm{yr}}^{-1}$. Current estimates for orbital lifetimes and space densities then imply steady-state captured populations of $\sim 10^2$ comets and $\sim 10^5$ `Oumuamua-like rocks, of which 0.033% are within 6au at any time.

5 pages, 3 figures, accepted for publication in MNRAS

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