Possibility of controlling solar system motion in the Galaxy

The possibility of developing a thruster for the solar system motion control in the Galaxy is considered. It is shown, that if a screen reflecting solar rays is positioned stationarily at some distance from the sun, the central symmetry of solar radiation in the sun-screen system will be violated and a force disturbing the sun motion will arise. The evaluation of screen surface density providing a stationary position of the screen is obtained on the assumption that the attractive forces and light pressure are equal. A disturbed motion of the solar system under the action of the above force is considered. It is shown that during one orbital period of the sun a radial deflection of the sun from its reference orbit by the value of some 10-12 parsec is possible. Lateral deviation of the sun by 4.4 parsec from its orbital plane is also possible, when the screen axis is normal to the orbital plane and has a constant orientation. The possibility of the earth transfer from the solar system onto a circular orbit of another star is shown.