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The main aim of photometrical observations of the asteroid 3200 Phaethon wassearching for its low-level cometary activity (possible coma and/or dust tail)in the pre-perihelion passage. We performed observational runs with telescopesranging from 0.61-m to 2-m and BVR color imaging. Three longer photometricseries were used for modeling of the 3D shape of Phaethon. The color indicesand size of the asteroid were estimated.

Photometric observations of the asteroid 3200 Phaethon using small and middle telescopes