(a) Show that the sum of the perihelion distance rmin and aphelion distance rmax of a planet is equal to 2a, where a is the semi-major axis of the orbit.
(a) Show that the sum of the perihelion distance rmin and aphelion distance rmax of a planet is equal to 2a, where a is the semi-major axis of the orbit.
(b) The Earth’s orbital eccentricity is 0.017 and its mean distance from the Sun (taken equal to the semi-major axis) is 1.496×1011m. Calculate the difference between the aphelion and perihelion distances of the Earth in kilometres.