
To solve this problem, we need to understand the dynamics of a planet's movement in an elliptical orbit according to Kepler's laws of planetary motion. The essential concept here is the conservation of angular momentum and energy.
The kinetic energy of a planet in an elliptical orbit varies with its distance from the Sun due to the conservation of angular momentum and energy. The key points in an elliptical orbit are:
According to the conservation of angular momentum:
\(mvr = \text{constant}\)
Here, \(m\) is the mass of the planet, \(v\) is the velocity, and \(r\) is the distance from the Sun.
At perihelion (A), the planet moves fastest, and at aphelion (C), it moves slowest. Therefore, the order of kinetic energies is:
Thus, the correct order of kinetic energies is:
KA > KB > KC
Therefore, the correct answer is KA > KB > KC.