Journal Article

Exploring S-type orbits in the Pluto–Charon binary system

S. M. Giuliatti Winter, O. C. Winter, A. H. Fernandes Guimarães and M. R. Silva

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 404, issue 1, pages 442-450
Published in print May 2010 | ISSN: 0035-8711
Published online April 2010 | e-ISSN: 1365-2966 | DOI:
Exploring S-type orbits in the Pluto–Charon binary system

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This work generates, through a sample of numerical simulations of the restricted three-body problem, diagrams of semimajor axis and eccentricity which defines stable and unstable zones for particles in S-type orbits around Pluto and Charon. Since we consider initial conditions with 0 ≤e≤ 0.99, we found several new stable regions. We also identified the nature of each one of these newly found stable regions. They are all associated to families of periodic orbits derived from the planar circular restricted three-body problem. We have shown that a possible eccentricity of the Pluto–Charon system slightly reduces, but does not destroy, any of the stable regions.

Keywords: Kuiper belt: general; minor planets, asteroids: general; planets and satellites: dynamical evolution and stability

Journal Article.  3617 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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