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   Mo[13.5]
   Di[14.5]
   Mi[15.5]
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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.