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3rd Austrian Hungarian Workshop
Rudolf Dvorak
Christoph Gamsjäger
A New determination of the Basic Frequencies in the Motion of the
Planets
In a secular theory of the motion of the planets the basic frequencies
are the ones of the nodes and the perhihelia. Besides the averaging
over the short periods for such theories
there are always truncations with respect to the small parameters
involved in the series
expansions of the solutions. Consequently a determination using the results
of numerical integrations of the full equations of motion is an interesting
approach. We present the results of the first analysis for a time
period covering 100 million years into the future and the past and compare them
to existing results.
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