OFFSET
0,2
COMMENTS
Minimum orbital eccentricity of a planet orbiting the sun with a 3:2 spin-orbit resonance (like Mercury) that allows one on it to see retrograde motion of the sun. In general, for a planet with a spin-orbit resonance k, there is retrograde motion if and only if the orbital eccentricity is greater than the unique real root of x^3 - 3*x^2 + (3 + 1/k^2)*x - (1 - 1/k^2) = 0.
The orbital eccentricity of Mercury is 0.205630, which is greater than 0.1910588914..., so there is retrograde motion of the sun on Mercury.
LINKS
EXAMPLE
Equals 0.19105889149184691057...
MATHEMATICA
First[RealDigits[Root[9*#^3 - 27*#^2 + 31*# - 5 &, 1], 10, 100]] (* Paolo Xausa, Jun 25 2024 *)
PROG
(PARI) solve(x=0, 1, 9*x^3 - 27*x^2 + 31*x - 5)
CROSSREFS
KEYWORD
AUTHOR
Jianing Song, May 17 2024
STATUS
approved
