Solution:
The escape velocity is given by the formula: $$ v_e = \sqrt{\frac{2GM}{R}} $$ where:
$v_e$ is the escape velocity
$G$ is the gravitational constant
$M$ is the mass of the celestial body
$R$ is the radius of the celestial body
Let:
$M_p$ be the mass of the planet
$R_p$ be the radius of the planet
$M_e$ be the mass of the Earth
$R_e$ be the radius of the Earth
$v_{ep}$ be the escape velocity of the planet
$v_{ee}$ be the escape velocity of the Earth
Given:
$M_p = 16 M_e$
$R_p = 4 R_e$
Escape velocity of Earth: $$ v_{ee} = \sqrt{\frac{2GM_e}{R_e}} $$ Escape velocity of the planet: $$ v_{ep} = \sqrt{\frac{2GM_p}{R_p}} $$ Ratio: $$ \frac{v_{ep}}{v_{ee}} = \frac{\sqrt{\frac{2GM_p}{R_p}}}{\sqrt{\frac{2GM_e}{R_e}}} = \sqrt{\frac{M_p R_e}{M_e R_p}} $$ Substitute the given values: $$ \frac{v_{ep}}{v_{ee}} = \sqrt{\frac{16M_e R_e}{M_e 4R_e}} = \sqrt{\frac{16}{4}} = \sqrt{4} = 2 $$ Therefore, the ratio of the escape velocity of the planet to the escape velocity of Earth is 2:1.
The correct answer is (2) 2:1.
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 \( a \in \mathbb{R} \) and \( A \) be a matrix of order \( 3 \times 3 \) such that \( \det(A) = -4 \) and \[ A + I = \begin{bmatrix} 1 & a & 1 \\ 2 & 1 & 0 \\ a & 1 & 2 \end{bmatrix} \] where \( I \) is the identity matrix of order \( 3 \times 3 \).
If \( \det\left( (a + 1) \cdot \text{adj}\left( (a - 1) A \right) \right) \) is \( 2^m 3^n \), \( m, n \in \{ 0, 1, 2, \dots, 20 \} \), then \( m + n \) is equal to:
In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.
According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,
On combining equations (1) and (2) we get,
F ∝ M1M2/r2
F = G × [M1M2]/r2 . . . . (7)
Or, f(r) = GM1M2/r2
The dimension formula of G is [M-1L3T-2].