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Allowed planetary orbits in the solar system
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 exopl...
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Published in: | Chaos, solitons and fractals solitons and fractals, 2008-06, Vol.36 (5), p.1273-1282 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | 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. |
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ISSN: | 0960-0779 1873-2887 |
DOI: | 10.1016/j.chaos.2006.07.056 |