The time period of a simple pendulum located at a height h = R above the Earth's surface is determined by the formula:
\[ T_1 = 2\pi \sqrt{\frac{\ell}{g_{\text{eff}}}} \]
Here, the effective acceleration due to gravity at height \(h = R\) is calculated as: \[ g_{\text{eff}} = \frac{GM}{(2R)^2} = \frac{g}{4} \]
Consequently, 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 a height \(h = 2R\), the effective acceleration due to gravity is: \[ g_{\text{eff}} = \frac{GM}{(3R)^2} = \frac{g}{9} \]
Thus, 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 these time periods is: \[ \frac{T_1}{T_2} = \sqrt{\frac{4}{9}} = \frac{2}{3} \]
This relationship can be expressed as: \[ 3T_1 = 2T_2 \]