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Horius Parry's avatar

Konstantin Meyl gives a modified version of the Titius-Bode law which gives good results for the planetary orbits and the moons of Jupiter

The average radius of the orbits is given by:

R(n) = R(0)Exp(n/K)

Where K is some constant dependent on the mass of the central object I think.

Derivation is via some sort of perturbation argument; orbits must be stable.

Page 256

https://avalonlibrary.net/Nikola_Tesla/Books/Meyl%20-%20Scalar%20Waves%20(First%20Tesla%20Physics%20Textbook).pdf

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adelaide tatnell's avatar

i would like more information about how the planets were spaced...

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