Suppose the gravitational force varies inversely as the nth power of distance. Then the time period of a planet in circular orbit of radius R around the sun will be proportional to\\
(1) $R ^ { \left( \frac { n + 1 } { 2 } \right) }$\\
(2) $R ^ { \left( \frac { n - 1 } { 2 } \right) }$\\
(3) $R ^ { n }$\\
(4) $\mathrm { R } ^ { \left( \frac { \mathrm { n } - 2 } { 2 } \right) }$