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Universal method of calculating perturbation function in numerical analysis theory of minor planet motion

I.A. Gerasimov, V.V. Chazov, D.A. Tagaeva

Moscow University Physics Bulletin 2000. 55. N 3. P. 64

  • Article
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.

Authors
I.A. Gerasimov, V.V. Chazov, D.A. Tagaeva
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Issue 3, 2000

Moscow University Physics Bulletin

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