Abstract:
The analysis of the properties of static spherical symmetric metric of the relativistic theory of gravitation in the vicinity of a singular sphere is done. It is shown that a massive particle in the nongeodesical radial motion may reach this sphere and be remained there in the rest. Basing on this property, it is inferred that the sphere formed by the massive particles can serve as the source of a singular metic in the relativistic theory of gravitation.