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Article overview
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Stellar encounters as the origin of distant solar system objects in highly eccentric orbits | Scott J. Kenyon
; Benjamin C. Bromley
; | Date: |
1 Dec 2004 | Journal: | Nature 432 (2004) 598 | Subject: | astro-ph | Abstract: | The discovery of Sedna places new constraints on the origin and evolution of our solar system. Here we investigate the possibility that a close encounter with another star produced the observed edge of the Kuiper belt, at roughly 50 AU, and the highly elliptical orbit of Sedna. We show that a passing star probably scattered Sedna from the Kuiper Belt into its observed orbit. The likelihood that a planet at 60-80 AU can be scattered into Sedna’s orbit is roughly 50%; this estimate depends critically on the geometry of the flyby. Even more interesting, though, is the roughly 10% chance that Sedna was captured from the outer disk of the passing star. Most captures have very high inclination orbits; detection of these objects would confirm the presence of extrasolar planets in our own Solar System. | Source: | arXiv, astro-ph/0412030 | Other source: | [GID 1103551] pmid15577903 | Services: | Forum | Review | PDF | Favorites |
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