Hill-type periodic orbits in the restricted three-body problem with oblate primaries

ASTROPHYSICS AND SPACE SCIENCE(2020)

Cited 1|Views2
No score
Abstract
We consider the planar circular restricted three body problem with oblate primaries. Using a suitable symplectic scaling and the Poincaré continuation method, we prove that in the proximity of any of the primaries there exist unstable periodic orbits.
More
Translated text
Key words
Restricted three-body problem,Oblate primaries,Poincare continuation method,Periodic orbits,Stability
AI Read Science
Must-Reading Tree
Example
Generate MRT to find the research sequence of this paper
Chat Paper
Summary is being generated by the instructions you defined