The time period of a simple pendulum at a height h = R above the earth’s surface is given by:
\[ T_1 = 2\pi \sqrt{\frac{\ell}{g_{\text{eff}}}} \]
where the effective acceleration due to gravity at a height \(h = R\) is: \[ g_{\text{eff}} = \frac{GM}{(2R)^2} = \frac{g}{4} \]
Thus, the time period at height \(R\) is: \[ T_1 = 2\pi \sqrt{\frac{\ell}{g/4}} = 2\pi \sqrt{\frac{4\ell}{g}} \]
Similarly, at height \(h = 2R\), the effective acceleration due to gravity is: \[ g_{\text{eff}} = \frac{GM}{(3R)^2} = \frac{g}{9} \]
Hence, the time period \(T_2\) is: \[ T_2 = 2\pi \sqrt{\frac{\ell}{g/9}} = 2\pi \sqrt{\frac{9\ell}{g}} \]
The ratio of the time periods is: \[ \frac{T_1}{T_2} = \sqrt{\frac{4}{9}} = \frac{2}{3} \]
This implies: \[ 3T_1 = 2T_2 \]