On the Restricted Three-Body Problem when the Mass Parameter is Small
Abstract
We study some aspects of the restricted three-body problem when the mass parameter μ is sufficiently small. First, we describe the global flow of the two-body rotating problem, μ=0, and we use it for the analysis of the collision and parabolic orbits when μ≳0. Also we show that for any fixed value of the Jacobian constant and for any ɛ>0, there exists a μ0>0 such that if the mass parameter μ∈[0,μ0], then the set of bounded orbits which are not contained in the closure of the set of symmetric periodic orbits has Lebesgue measure less than ɛ.
- Publication:
-
Celestial Mechanics
- Pub Date:
- October 1982
- DOI:
- 10.1007/BF01230662
- Bibcode:
- 1982CeMec..28...83L
- Keywords:
-
- Existence Theorems;
- Three Body Problem;
- Collisions;
- Manifolds (Mathematics);
- Mass;
- Orbits;
- Two Body Problem;
- Astronomy