The Capture of Centaurs as Trojans
arXiv:astro-ph/0511791 · doi:10.1111/j.1745-3933.2006.00131.x
Abstract
Large scale simulations of Centaurs have yielded vast amounts of data, the analysis of which allows interesting but uncommon scenarios to be studied. One such rare phenomenon is the temporary capture of Centaurs as Trojans of the giant planets. Such captures are generally short (10 kyr to 100 kyr), but occur with sufficient frequency (about 40 objects larger than 1 km in diameter every Myr) that they may well contribute to the present-day populations. Uranus and Neptune seem to have great difficulty capturing Centaurs into the 1:1 resonance, while Jupiter captures some, and Saturn the most (80 %). We conjecture that such temporary capture from the Centaur population may be the dominant delivery route into the Saturnian Trojans. Photometric studies of the Jovian Trojans may reveal outliers with Centaur-like as opposed to asteroidal characteristics, and these would be prime candidates for captured Centaurs.
5 pages, 2 figures, submitted to MNRAS (Letters)
References in corpus (8)
- Simulations of the Population of Centaurs I: The Bulk Statistics
- Population and Size Distribution of Small Jovian Trojan Asteroids
- Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances
- On the origin of the Trojan asteroids: Effects of Jupiter's mass accretion and radial migration
- Simulations of the Population of Centaurs II: Individual Objects
- Ultra Deep Survey for Irregular Satellites of Uranus: Limits to Completeness
- Cartography for Martian Trojans
- Asteroids in the Inner Solar System II - Observable Properties
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- Astrocladistics of the Jovian Trojan Swarms
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- The Stability of Uranus Trojans Over the Age of the Solar System