A planet in another solar system orbits a star with a mass of 4.0×1030 kg. At one point in its orbit it is 250×106 km from the star and is moving at 35 km/s. Take the universal gravitational constant to be 6.67×10−11 Nm2/s2 and calculate the semi-major axis of the planet's orbit. The result is:
(A) 79×106 km
(B) 160×106 km
(C) 290×106 km
(D) 320×106 km