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

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  • Craig B. Agnor

    (Center for the Origin, Dynamics and Evolution of Planets, University of California)

  • Douglas P. Hamilton

    (University of Maryland at College Park)

Abstract

Triton's capture Unique among the Solar System's large satellites, Triton orbits Neptune in the direction opposite to the planet's spin. Triton's circular orbit is also tilted significantly from Neptune's equator. These facts suggest that the satellite once orbited the Sun before capture by Neptune, but previous models of the capture required improbable events. Craig Agnor and Douglas Hamilton have developed a more natural explanation. In this model, Triton was once a member of a binary that may have been rather like Pluto and its largest moon Charon. The pair strayed too close to Neptune and were torn apart; the companion escaped, but left Triton behind. The cover depicts this encounter. Neptune is orbited by primordial satellites that would not have survived long after Triton's capture. (Graphic based on planetary and satellite maps provided by Steve Albers, Jerry Gardner, James Hastings-Trew, Constantine Thomas and NOAA's ‘Science on a Sphere’ project.)

Suggested Citation

  • Craig B. Agnor & Douglas P. Hamilton, 2006. "Neptune's capture of its moon Triton in a binary–planet gravitational encounter," Nature, Nature, vol. 441(7090), pages 192-194, May.
  • Handle: RePEc:nat:nature:v:441:y:2006:i:7090:d:10.1038_nature04792
    DOI: 10.1038/nature04792
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    Cited by:

    1. Benjamin Proudfoot & Darin Ragozzine, 2022. "The formation of Haumea and its family via binary merging," Nature Communications, Nature, vol. 13(1), pages 1-8, December.

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