Three families of trajectories in vicinity of the 1:1 mean-motion resonance are discussed: quasi-circular trajectories, ”stable chaos” trajectories, trajectories which exits from the resonance. The dependence corresponding initial conditions on planet’s mass is investigated, as well the complicated eccentricity evolution in the region of ”stable chaos”.
Original languageEnglish
Title of host publicationProceedings “Resonances, stabilization, and stable chaos in hierarchical triple systems, Sept. 8-13, 2008”, 2009, p.8-15
PublisherKisarazu
Pages100 стр., 8-15
Number of pages8
ISBN (Print)978-4-485-30105-0
StatePublished - 2009

    Research areas

  • restricted three-body problem, resonant orbits, chaos

ID: 4441028