Correct answer: R^((n+1)/2)
The period of a planet in a circular orbit is derived from Kepler's third law, which states that the square of the period is proportional to the cube of the semi-major axis of the orbit. When gravitational attraction is inversely proportional to the nth power of the separation, the relationship modifies to show that the period is proportional to R raised to the power of (n+1)/2, reflecting the balance between gravitational force and centripetal force.