The time period \(T\) of a simple pendulum is related to the acceleration due to gravity \(g\) by the formula:
\[ T = 2\pi \sqrt{\frac{L}{g}} \]
where \(L\) is the length of the pendulum and \(g\) is the acceleration due to gravity.
At a height \(h = 2R\) from the surface of the Earth, the acceleration due to gravity \(g'\) is given by:
\[ g' = g \left( \frac{R}{R + h} \right)^2 \]
Substituting \(h = 2R\):
\[ g' = g \left( \frac{R}{3R} \right)^2 = \frac{g}{9} \]
Therefore, the new value of gravitational acceleration at height \(h = 2R\) is \(\frac{g}{9}\).
The time period \(T\) of a pendulum is related to the length \(L\) and the acceleration due to gravity \(g\) by:
\[ T = 2\pi \sqrt{\frac{L}{g}} \]
At height \(h = 2R\), the new time period \(T'\) will be:
\[ T' = 2\pi \sqrt{\frac{L'}{g'}} \]
Since the time period remains 2 seconds, we equate the time periods:
\[ 2 = 2\pi \sqrt{\frac{L'}{g/9}} \]
Squaring both sides:
\[ 1 = \pi^2 \frac{L'}{g} \]
Solving for \(L'\):
\[ L' = \frac{g}{\pi^2} \]
Substitute \(g = \pi^2 \, \text{m/s}^2\) into the equation:
\[ L' = \frac{\pi^2}{9\pi^2} = \frac{1}{9} \, \text{m} \]
Thus, the length of the second's pendulum at a height \(h = 2R\) is \(\frac{1}{9} \, \text{m}\).