| Summary: | The paper is devoted to elaboration of the new optimized methods, algorithms and programs for the solution of problems of the remote control of near-earth space (CS), which are related to investigation of cosmic objects (CO) based on the photometric and coordinate measurements. It is shown, that for these determination of satellite's rotation period around center of mass, the orientation of rotation axis, and also its color, polarization and others characteristics can be used. The main principles of a system of the CO identification based on their light curves are elaborated. A new algorithm of CO orbit determination using the network station data is created. Its accuracy is by 3-4 orders at magnitude higher than that of algorithms based on the well-known methods of celestial mechanics.
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