Contact Geometry of the Restricted Three-Body Problem on S2

Abstract

We study the contact geometry of the connected components of the energy hypersurface, in the symmetric restricted 3-body problem on S2, for a specific type of motion of the primaries. In particular, we show that these components are of contact type for all energies below the first critical value and slightly above it. We prove that these components, suitably compactified using a Moser-type regularization are contactomorphic to RP3 with its unique tight contact structure or to the connected sum of two copies of it, depending on the value of the energy. We exploit Taubes' solution of the Weinstein conjecture in dimension three, to infer the existence of periodic orbits in all these cases.

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