We prove the existence of chaotic almost collision orbits of the plane restricted elliptic 3-body problem with small mass ratio and eccentricity shadowing chains of collision orbits of Kepler's problem. The proof is based on the dynamics of random compositions of nearly integrable symplectic maps.
No takes yet. Share an insight, caveat, or question.
Sergey Bolotin (2006) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: