Motion of particles in a centrally symmetric field in the relativistic theory of gravitation

The paper considers the displacement of the pericenter and the revolution period of a particle orbiting in the spherically symmetric metric that in the relativistic theory of gravitation generalizes the harmonic interval of Fock and contains a second constant (proportional to the radius of the central body and with a dependence on its structure). It is shown that this constant occurs explicitly in the expressions for both effects and, therefore, can in principle be determined from the motion of particles.