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Nature 439, 924-925 (23 February 2006) | doi:10.1038/439924a; Published online 22 February 2006

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Planetary science: Pluto's expanding brood

Richard P. Binzel1

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Pluto is no lone ranger in the farthest expanses of the Solar System — its travelling companions now number three. And if Pluto can have so many, why shouldn't other objects in the distant, icy Kuiper belt?

Once thought to be a solitary denizen of the outer reaches of the Solar System, Pluto — which piqued our curiosity in 1978 with the discovery of its large satellite, Charon1 — is becoming ever more intriguing. In fact, the relative sizes of Pluto and Charon (Charon's diameter of around 1,200 kilometres is just over half that of Pluto's) means they are a 'double planet', orbiting a mutual centre of gravity, or barycentre, outside the surface of Pluto.

  1. Richard P. Binzel is in the Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.
    Email: rpb@mit.edu

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