On integrating the evolutionary equations in the Restricted Three-Body Problem with variable masses

We consider a generalized case of a satellite version of the restricted three-body problem when two points P0 and P1 form a binary system, losing the mass due to the corpuscular and photon radiation. We assume that the points masses vary isotropically with different rates with the only
restriction that their total mass reduces according to so-called joint Meshcherskii law. In this case equations of the relative motion of the points P0, P1 are integrable and their general solution can be written in symbolic form.