To solve this problem it is necessary to apply the concepts related to Kepler's second law and the conservation of angular momentum.
Kepler's second law tells us that the vector radius that unites a planet and the sun sweeps equal areas at equal times, that is, when the planet is farther from the sun, the speed at which it travels is less than when it is close to the sun.
The angular momentum is defined as
Where,
m= mass
r = Radius
v = Velocity
For conservation of angular momentum
Therefore the corresponding distance at apogee is