(b) From Kepler’s third law of planetary motion
$\ \ \ \ \ \ \ \ \ \ \ \ \ T^{2} \propto R^{3}$
$Given,\ T_{1} = 1,\ T_{2} = 8,\ R_{1} = R$
$\therefore\ \ \ \ \ \ \ \frac{T_{1}^{2}}{T_{2}^{2}} = \frac{R_{1}^{3}}{R_{2}^{3}}$
$\ \ \ \ \ \ \ \ \ R_{2}^{3} = R_{1}^{3}\frac{{\ \ T}_{2}^{2}}{T_{1}^{2}}\ \ \ $
$\ \ \ \ \ \ \ \ \ R_{2}^{3} = R_{1}^{3} \times (8)^{2}$
$\ \ \ \ \ \ \ \ \ R_{2}^{3} = R^{3} \times \left( 2^{3} \right)^{2}$
$\Rightarrow \ \ \ R_{2} = R \times 4 = 4R$