by John on (#6C8N2)
Suppose a planet is in an elliptical orbit around the sun with semimajor axis a and semiminor axis b. Then the average distance of the planet to the sun over time equals a(1 + e^2/2) where the eccentricity e satisfies e^2 = 1 - b^2/a^2. You can find a proof of this statement in [1]. [...]The post Set of orbits with the same average distance to sun first appeared on John D. Cook.