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Allowed planetary orbits in the solar system

Author

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  • Pintr, P.
  • Peřinová, V.
  • Lukš, A.

Abstract

A new law of the Titius–Bode type for planetary distances from the Sun is proposed. These distances for each planet are determined using appropriate nodal circle of a vibrating membrane. Regularities in the distribution of bodies in the solar system and in the systems of giant planets and some exoplanets are pointed out.

Suggested Citation

  • Pintr, P. & Peřinová, V. & Lukš, A., 2008. "Allowed planetary orbits in the solar system," Chaos, Solitons & Fractals, Elsevier, vol. 36(5), pages 1273-1282.
    • Handle: RePEc:eee:chsofr:v:36:y:2008:i:5:p:1273-1282
    DOI: 10.1016/j.chaos.2006.07.056
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    References listed on IDEAS

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    1. El Naschie, M.S., 2006. "Topics in the mathematical physics of E-infinity theory," Chaos, Solitons & Fractals, Elsevier, vol. 30(3), pages 656-663.
    2. de Oliveira Neto, Marçal, 2006. "Pythagoras’ celestial spheres in the context of a simple model for quantization of planetary orbits," Chaos, Solitons & Fractals, Elsevier, vol. 30(2), pages 399-406.
    3. Oliveira Neto, Marçal de, 2005. "Using the dimensionless Newton gravity constant α¯G to estimate planetary orbits," Chaos, Solitons & Fractals, Elsevier, vol. 24(1), pages 19-27.
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    Cited by:

    1. Krot, Alexander M., 2009. "A statistical approach to investigate the formation of the solar system," Chaos, Solitons & Fractals, Elsevier, vol. 41(3), pages 1481-1500.

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