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Abstract
We propose a new dynamical model for capture of irregular moons which identifies chaos as the essential feature responsible for initial temporary gravitational trapping within a planet's Hill sphere. The key point is that incoming potential satellites get trapped in chaotic orbits close to “sticky” KAM tori in the neighbourhood of the planet, possibly for very long times, so that the chaotic layer largely dictates the final orbital properties of captured moons.
Original language | English |
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Title of host publication | Order and Chaos in Stellar and Planetary Systems |
Editors | Gene G. Byrd, Konstantin V. Kholshevnikov, Aleksandr A. Myllari, Igor' I. Nikiforov, Victor V. Orlov |
Publisher | Astronomical Society of the Pacific |
Pages | 80-85 |
Number of pages | 6 |
ISBN (Electronic) | 9781583812518 |
ISBN (Print) | 1583811729 |
Publication status | Published - 1 Jan 2004 |
Publication series
Name | Astronomical Society of the Pacific Conference Series |
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Publisher | Astronomical Society of the Pacific |
Volume | 316 |
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Dive into the research topics of 'Dynamics of capture in the restricted three-body problem'. Together they form a unique fingerprint.Activities
- 1 Visiting an external academic institution
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Utah State University
Andrew Burbanks (Visiting researcher)
27 May 2003 → 7 Jun 2003Activity: Visiting an external organisation types › Visiting an external academic institution