Non-restricted double-averaged three body problem in Hill's case
From MaRDI portal
Publication:4110651
DOI10.1007/BF01229100zbMath0342.70009MaRDI QIDQ4110651
Publication date: 1976
Published in: Celestial Mechanics (Search for Journal in Brave)
Celestial mechanics (70F15) (n)-body problems (70F10) Collision of rigid or pseudo-rigid bodies (70F35)
Related Items
Harrington's Hamiltonian in the stellar problem of three bodies: Reductions, relative equilibria and bifurcations ⋮ The Keplerian regime of charged particles in planetary magnetospheres ⋮ Quasi‐Periodic Almost‐Collision Orbits in the Spatial Three‐Body Problem ⋮ Secular and tidal evolution of circumbinary systems ⋮ Analysis of the orbital evolution of exoplanets ⋮ Regular and singular reductions in the spatial three-body problem ⋮ On the co-existence of maximal and whiskered tori in the planetary three-body problem ⋮ Tidal evolution of hierarchical and inclined systems ⋮ The phase-space architecture in extrasolar systems with two planets in orbits of high mutual inclination ⋮ Investigation of the restricted problem of three bodies of variable masses using computer algebra ⋮ Aspects of the planetary Birkhoff normal form ⋮ INTERMEDIATE-MASS BLACK HOLES ⋮ Secular resonances between bodies on close orbits: a case study of the Himalia prograde group of Jovian irregular satellites ⋮ Flow reconstruction and invariant tori in the spatial three-body problem ⋮ Circulating, eccentric periodic orbits at the Moon ⋮ Kustaanheimo-Stiefel regularization and the quadrupolar conjugacy ⋮ Quasi-periodic solutions of the spatial lunar three-body problem ⋮ Quasiperiodic motions in the planar three-body problem ⋮ Canonical coordinates for the planetary problem ⋮ Reduction of some perturbed Keplerian problems ⋮ Global Kolmogorov tori in the planetary \(N\)-body problem. Announcement of result
Cites Work
