Аннотация:We present the results of photometrical measurements for two near-Earth asteroids and one Centaur group asteroid which were observed in 2008─2010 years with the 1-m Simeiz telescope of Institute of Astronomy RAS. The most precise value of the rotation period of asteroid 2002 NP1 was derived as 0.24626 day, the colour-index V − Rc = 0.55 is derived; the Q taxonomic class of 5786 Talos was found; the detected brightness variability of the asteroid 2005 WY3 is due to its rotation with a period 0.83 or 0.62 days.
