Step 1: Kepler's third law
\[
T^2 \propto R^3
\]
Step 2: Calculate the new time period
\[
\left( \frac{T_2}{T_1} \right)^2 = \left( \frac{R_2}{R_1} \right)^3
\]
Substitute values:
\[
T_2 = \left( \frac{3R}{R} \right)^{3/2} \times 1
\]
\[
= 3\sqrt{3} \text{ years}
\]
The new time period is \( 3\sqrt{3} \) years.