If the height of a satellite from the earth is negligible in comparison of the radius of the earth R, the orbital velocity of the satellite is
(A) gR
(B) (gR / 2)
(C) √(g/R)
(D) √(gR)
Correct option: (D) √(gR)
Explanation:
Orbital velocity near to earth = [(escape velocity) / √2]
V = (Ve / √2)
V = [{√(2gr)} / √2] = √(gR)