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We present the results of the investigation of one possible mechanism which can be the source of meteoroids with the hyperbolic orbital velocity, the mutual collisions of the Oort cloud objects, the Kuiper belt objects, or the Main asteroid belt, or their collisions with other populations of small solar system bodies. In our study we used model orbits of the Oort cloud objects, the Classical objects of the Kuiper belt, and the Main asteroid belt objects with different values of the semi-major axis and studied the orbital behaviour of their fragments after the collision with other small bodies, e. g. bodies on orbits similar to the Kreutz cometary orbits. Depending on its direction, the fragments will migrate into the inner or outer part of the solar system with the different orbital velocity.