http://arxiv.org/abs/1910.06338
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 $\sim10^2$ comets and $\sim10^5$Oumuamua-like rocks.
T. Hands and W. Dehnen
Wed, 16 Oct 19
42/56
Comments: 5 pages, 3 figures, submitted to MNRAS