Dynamics of capture in the restricted three-body problem

S. Astakhov, A. Burbanks, S. Wiggins, D. Farrelly

Research output: Chapter in Book/Report/Conference proceedingChapter (peer-reviewed)peer-review

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 languageEnglish
Title of host publicationOrder and Chaos in Stellar and Planetary Systems
EditorsGene G. Byrd, Konstantin V. Kholshevnikov, Aleksandr A. Myllari, Igor' I. Nikiforov, Victor V. Orlov
PublisherAstronomical Society of the Pacific
Pages80-85
Number of pages6
ISBN (Electronic)9781583812518
ISBN (Print)1583811729
Publication statusPublished - 1 Jan 2004

Publication series

NameAstronomical Society of the Pacific Conference Series
PublisherAstronomical Society of the Pacific
Volume316

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