According to Kepler's law of periods
$T^{2}\,\propto\,R^{3}$
So,$\,\Rightarrow \, \frac{T_{1}}{T_{2}}=\left(\frac{R_{1}}{R_{2}}\right)^{\frac{3}{2}}$
$\Rightarrow \, \frac{T}{T_{2}}=\left(\frac{R}{9R}\right)^{\frac{3}{2}}\,=\frac{1}{27}\,\left[\because \,T_{1}=T\right]$
$T_{2}=27T$