On the period of the periodic orbits of the restricted three body problem

Abstract

We will show that the period $T$ of a closed orbit of the planar circular restricted three-body problem (viewed on rotating coordinates) depends on the region it encloses. Roughly speaking, we show that, $2T=k\pi +{\int }_{\Omega }g$ where $k$ is an integer, $\Omega$ is the region enclosed by the periodic orbit and $g:{\mathbb{R}}^2\to \mathbb{R}$ is a function that only depends on the constant $C$ known as the Jacobian integral; it does not depend on $\Omega$. This theorem has a Keplerian flavor in the sense that it relates the period with the space "swept" by the orbit. As an application, we prove that there is a neighborhood around $L_4$ such that every periodic solution contained in this neighborhood must move clockwise. The same result holds true for $L_5$.

5 figures

References in corpus (2)

• Rotating Drops with Helicoidal Symmetry
• Constant Speed Ramps