Annotation
A second approximation has been derived for the theory of motion of solar system bodies based on a universal method for computing the perturbation function. The results of processing a 30-year series of photographic observations of selected minor planets have been presented.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
I.A. Gerasimov, V.V. Chazov, D.A. Tagaeva
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia