The kinetic energies of a planet 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 S as shown in the figure.Then

A

$$K_{B}>K_{A}> K_{C}$$

B

$$K_{B}<K_{A}< K_{C}$$

C

$$K_{A}>K_{B}> K_{C}$$

D

$$K_{A}<K_{B}<K_{C}$$