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

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

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006natur.441..192a&link_type=abstract

Nature, Volume 441, Issue 7090, pp. 192-194 (2006).

Physics

44

Scientific paper

Triton is Neptune's principal satellite and is by far the largest retrograde satellite in the Solar System (its mass is ~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. Existing models 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 ~103-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.

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