Resonant motion in the restricted three-body problem
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Publication:687250
DOI10.1007/BF00699733zbMath0780.70004OpenAlexW4246105466MaRDI QIDQ687250
Publication date: 6 February 1994
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf00699733
Related Items (14)
Constructing motion primitive sets to summarize periodic orbit families and hyperbolic invariant manifolds in a multi-body system ⋮ Critical point families at the 3:1 resonance ⋮ The integrable cases of the three-body problem at second-order resonance under the high oblateness of the central body ⋮ Dynamic expansion points: an extension to Hadjidemetriou's mapping method ⋮ On the measure of the structure around the last KAM torus before and after its break-up ⋮ A symplectic mapping approach to the study of the stochasticity in asteroidal resonances ⋮ Mapping and dynamical systems ⋮ On the period of the periodic orbits of the restricted three body problem ⋮ Explicit symplectic integrator for highly eccentric orbits ⋮ Networks and Bifurcations of Eccentric Orbits in Exoplanetary Systems ⋮ Wisdom system: dynamics in the adiabatic approximation ⋮ Origin and continuation of \(3/2, 5/2, 3/1, 4/1\) and \(5/1\) resonant periodic orbits in the circular and elliptic restricted three-body problem ⋮ Inclined asymmetric librations in exterior resonances ⋮ Chaotic Di?usion of Asteroids
Cites Work
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- On the dynamics in the asteroids belt. I: General theory
- On the dynamics in the asteroids belt. II: Detailed study of the main resonances
- The elliptic restricted problem at the 3:1 resonance
- On symmetrical planetary corotations
- Regular and stochastic motion
- On the relation between resonance and instability in planetary systems
- High-order resonances in the restricted three-body problem
- The present status of periodic orbits
- BURRAU'S PROBLEM OF THREE BODIES
- Stability of periodic orbits in the elliptic, restricted three-body problem.
- Periodic collision orbits in the elliptic restricted three-body problem
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