Orbital Period Ratios and Fibonacci Numbers in Solar Planetary and Satellite Systems and in Exoplanetary Systems

Vladimir Pletser

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arXiv · 1803.02828

Orbital Period Ratios and Fibonacci Numbers in Solar Planetary and Satellite Systems and in Exoplanetary Systems

Vladimir Pletser

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Abstract

It is shown that orbital period ratios of successive secondaries in the Solar planetary and giant satellite systems and in exoplanetary systems are preferentially closer to irreducible fractions formed with Fibonacci numbers between 1 and 8 than to other fractions, in a ratio of approximately 60% to 40%. Furthermore, if sets of minor planets are chosen with gradually smaller inclinations and eccentricities, the proximity to Fibonacci fractions of their period ratios with Jupiter or Mars$'$ period tends to increase. Finally, a simple model explains why the resonances with ratios of orbital periods $P_{1}$ and $P_{2}$ of successive secondaries being equal to ratio of small integers $p$ and $(p+q)$, $P_{1}/P_{2}=p/(p+q)$, are stronger and more commonly observed.

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Vladimir Pletser. 2018-03-07. Orbital Period Ratios and Fibonacci Numbers in Solar Planetary and Satellite Systems and in Exoplanetary Systems. https://arxiv.org/abs/1803.02828

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