From rotations and inclinations to zero configurational velocity surfaces I. A natural rotating coordinate system
From MaRDI portal
Publication:3341960
DOI10.1007/BF01241046zbMath0549.70003MaRDI QIDQ3341960
Publication date: 1984
Published in: Celestial Mechanics (Search for Journal in Brave)
Related Items (11)
Global geometry of non-planar 3-body motions ⋮ Zero velocity hypersurfaces for the general three-dimensional three-body problem ⋮ Natural dynamical reduction of the three-body problem ⋮ From rotations and inclinations to zero configurational velocity surfaces, II. The best possible configurational velocity surfaces ⋮ Constant inclination solutions in the three-body problem ⋮ The masses in an isosceles solution of the three-body problem ⋮ Saari's homographic conjecture of the three-body problem ⋮ Restriction on the motion of a solid in a gravitational field ⋮ Stability criteria for hierarchical triple systems ⋮ A century-long loop. ⋮ Hill regions of charged three-body systems
Cites Work
- The manifold structure for collision and for hyperbolic-parabolic orbits in the n-body problem
- On the manifolds of total collapse orbits and of completely parabolic orbits for the n-body problem
- \(N\)-body spatial parabolic orbits asymptotic to collinear central configurations
- Restrictions on the Motion of the Three-Body Problem
- Hill regions for the general three-body problem
- TheN-body problem of celestial mechanics
- Unnamed Item
- Unnamed Item
This page was built for publication: From rotations and inclinations to zero configurational velocity surfaces I. A natural rotating coordinate system
