The capture of Centaurs as Trojans

被引:42
作者
Horner, J
Evans, NW
机构
[1] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland
[2] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
关键词
comets : general; minor planets; asteroids; planets and satellites : general; solar system : general;
D O I
10.1111/j.1745-3933.2006.00131.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Large-scale simulations of Centaurs have yielded vast numbers 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 (10-100 kyr), but occur with sufficient frequency (similar to 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 (similar to 80 per cent). 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.
引用
收藏
页码:L20 / L23
页数:4
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