The kinetic energies of planets in an elliptical orbit about the Sun, at positions A, B and C are \(K_{A}\), \(K_{B}\) and \(K_{C}\), respectively. AC is the major axis and SB is perpendicular to AC at the position of the Sun as shown in figure. Then
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A planet moves fastest near the Sun and slowest farthest from it, so kinetic energy decreases with distance from the Sun.