Neptune's capture of its moon Triton in a binary-planet gravitational encounter

被引:214
作者
Agnor, CB
Hamilton, DP
机构
[1] Univ Calif Santa Cruz, Dept Earth Sci, Ctr Origin Dynam & Evolut Planets, Santa Cruz, CA 95064 USA
[2] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
关键词
D O I
10.1038/nature04792
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Triton is Neptune's principal satellite and is by far the largest retrograde satellite in the Solar System ( its mass is similar to 40 per cent greater than that of Pluto). Its inclined and circular orbit lies between a group of small inner prograde satellites and a number of exterior irregular satellites with both prograde and retrograde orbits. This unusual configuration has led to the belief that Triton originally orbited the Sun before being captured in orbit around Neptune(1-3). Existing models(4-6) for its capture, however, all have significant bottlenecks that make their effectiveness doubtful. Here we report that a three-body gravitational encounter between a binary system (of similar to 10(3)-kilometre-sized bodies) and Neptune is a far more likely explanation for Triton's capture. Our model predicts that Triton was once a member of a binary with a range of plausible characteristics, including ones similar to the Pluto - Charon pair.
引用
收藏
页码:192 / 194
页数:3
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