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.
Net gravitational force at the center of a square is found to be \( F_1 \) when four particles having masses \( M, 2M, 3M \) and \( 4M \) are placed at the four corners of the square as shown in figure, and it is \( F_2 \) when the positions of \( 3M \) and \( 4M \) are interchanged. The ratio \( \dfrac{F_1}{F_2} = \dfrac{\alpha}{\sqrt{5}} \). The value of \( \alpha \) is 
