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 on to orbits akin to those of known long-period comets. This suggests that some of these comets could be of extrasolar origin, in particular inactive ones. Assuming ISOs follow the local stellar velocity distribution, we infer a volume capture rate of 0.051 au(3) yr(-1). Current estimates for orbital lifetimes and space densities then imply steady-state captured populations of similar to 10(2) comets and similar to 10(5) 'Oumuamua-like rocks, of which 0.033 per cent are within 6 au at any time.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Physik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 530 Physik |
ISSN: | 0035-8711 |
Sprache: | Englisch |
Dokumenten ID: | 89414 |
Datum der Veröffentlichung auf Open Access LMU: | 25. Jan. 2022, 09:30 |
Letzte Änderungen: | 25. Jan. 2022, 09:30 |