Abstract
The deviations under radiation pressure influence were calculated for three asteroids 308635 (2005 YU55), 367943 Duende (2012 DA14) and 357439 (2004 BL86) that had a close encounter with the Earth. Calculations were made for different values of the assumed albedo of the asteroids. Deviations in orbital motion of the asteroids before the next close encounter with the Earth are also presented.
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