The Yarkovsky effect in generalized photogravitational 3-body problem

Here a generalization of photogravitational restricted 3-body problem to the case of influence of Yarkovsky effect is presented, which is known as the reason of additional infinitesimal acceleration of small bodies in the space (due to anisotropic re-emission of absorbed energy from the sun, and other stellar sources). id is supposed to move under the influence of gravitational forces from 2 massive bodies (which are rotating around their common center of masses on Keplerʹs trajectories), as well as under the influence of pressure of light from both the primaries. ing the ODE system of motion, we explore the existence of equilibrium points for a small body (asteroid) in the case when the 2-nd primary is non-oblate spheroid. h a case, the existence of maximally 256 different non-planar libration points in generalized photogravitational restricted 3-body problem when we take into consideration even a small Yarkovsky effect is proved.