Step 1: Formula for the time period of a simple pendulum.
\[
T = 2\pi \sqrt{\frac{L}{g}}
\]
where \( g \) is the acceleration due to gravity.
Step 2: Relation of \( g \) with planet’s mass and radius.
\[
g = \frac{GM}{R^2}.
\]
Let \( g_E \) be the acceleration due to gravity on Earth and \( g_P \) on the new planet.
Given: \[ M_P = 4M_E, \quad R_P = 2R_E. \] Thus, \[ g_P = \frac{G M_P}{R_P^2} = \frac{G(4M_E)}{(2R_E)^2} = \frac{4GM_E}{4R_E^2} = g_E. \]
Step 3: Compare time periods.
Since \( g_P = g_E \),
\[
T_P = 2\pi \sqrt{\frac{L}{g_P}} = 2\pi \sqrt{\frac{L}{g_E}} = T_E.
\]
Hence, **time period remains the same.**
Step 4: Analyze statements.
- Assertion (A): “Time period remains same” → ✅ True (since \( g_P = g_E \)).
- Reason (R): “Mass of the pendulum remains unchanged” → although true as a physical fact, **it is not the reason** why the time period remains same — time period depends on \( g \), not on the pendulum’s mass.
\[ \boxed{\text{(A) is true but (R) is false.}} \]
A small point of mass \(m\) is placed at a distance \(2R\) from the center \(O\) of a big uniform solid sphere of mass \(M\) and radius \(R\). The gravitational force on \(m\) due to \(M\) is \(F_1\). A spherical part of radius \(R/3\) is removed from the big sphere as shown in the figure, and the gravitational force on \(m\) due to the remaining part of \(M\) is found to be \(F_2\). The value of the ratio \( F_1 : F_2 \) is: 
Match the LIST-I with LIST-II
\[ \begin{array}{|l|l|} \hline \text{LIST-I} & \text{LIST-II} \\ \hline \text{A. Gravitational constant} & \text{I. } [LT^{-2}] \\ \hline \text{B. Gravitational potential energy} & \text{II. } [L^2T^{-2}] \\ \hline \text{C. Gravitational potential} & \text{III. } [ML^2T^{-2}] \\ \hline \text{D. Acceleration due to gravity} & \text{IV. } [M^{-1}L^3T^{-2}] \\ \hline \end{array} \]
Choose the correct answer from the options given below:
Let \( f : \mathbb{R} \to \mathbb{R} \) be a twice differentiable function such that \[ (\sin x \cos y)(f(2x + 2y) - f(2x - 2y)) = (\cos x \sin y)(f(2x + 2y) + f(2x - 2y)), \] for all \( x, y \in \mathbb{R}. \)
If \( f'(0) = \frac{1}{2} \), then the value of \( 24f''\left( \frac{5\pi}{3} \right) \) is: