The minimum speed at which an object is thrown to escape the gravitational pull of the moon is known as the escape velocity. The escape velocity \( v_e \) is given by the formula: \[ v_e = \sqrt{\frac{2GM}{R}} \] Where:
\( G \) is the gravitational constant (\( 6.67 \times 10^{-11} \, \text{Nm}^2/\text{kg}^2 \)),
\( M \) is the mass of the moon (\( 7.35 \times 10^{22} \, \text{kg} \)),
\( R \) is the radius of the moon (\( 1.74 \times 10^6 \, \text{m} \)).
Substituting the known values: \[ v_e = \sqrt{\frac{2 \times 6.67 \times 10^{-11} \times 7.35 \times 10^{22}}{1.74 \times 10^6}} \] \[ v_e = \sqrt{\frac{9.79 \times 10^{12}}{1.74 \times 10^6}} = \sqrt{5.63 \times 10^6} \] \[ v_e \approx 2370 \, \text{m/s} \quad \text{or} \quad 2.3 \, \text{km/s} \] Thus, the minimum speed required is approximately \( 2.3 \, \text{km/s} \).
The correct option is (E) : \(2.3 \, \text{km/s}\)
Answer: 2.3 km/s
Explanation:
To ensure an object escapes the Moon’s gravitational field, it must be projected with a speed equal to or greater than the escape velocity.
The escape velocity is given by the formula:
$$ v_e = \sqrt{\frac{2GM}{R}} $$ where:
- $G$ is the universal gravitational constant
- $M$ is the mass of the Moon
- $R$ is the radius of the Moon
Using the known values for the Moon,
$$ v_e \approx 2.3 \, \text{km/s} $$ Therefore, the minimum speed required is 2.3 km/s.
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:
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: 