The kinetic energies of a planet in an elliptical orbit around the Sun, at positions A, B and C are KA, KB and KC respectively. AC is the major axis and SB is perpendicular to AC at the position of the Sun S, as shown in the figure. Then:
1. | \(K_A <K_B< K_C\) | 2. | \(K_A >K_B> K_C\) |
3. | \(K_B <K_A< K_C\) | 4. | \(K_B >K_A> K_C\) |