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A body is projected upwards with a veloc...

A body is projected upwards with a velocity of `3 xx 11.2 "km s"^(-1)` from the surface of earth. What will be the velocity of the body when it escapes from the gravitational pull of earth ?

A

`11.2 "km s"^(-1)`

B

`sqrt(2) xx 11.2 "km s"^(-1)`

C

`sqrt(3) xx 11.2 "km s"^(-1)`

D

`sqrt(8) xx 11.2 "km s"^(-1)`

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem, we will use the principle of conservation of energy. The total mechanical energy (kinetic + potential) of the body when it is projected upwards should equal the total mechanical energy when it escapes the gravitational pull of the Earth. ### Step-by-Step Solution: 1. **Identify Given Values:** - Initial velocity of the body, \( v_i = 3 \times 11.2 \, \text{km/s} \) - Escape velocity from the surface of the Earth, \( v_e = 11.2 \, \text{km/s} \) 2. **Calculate Initial Velocity:** \[ v_i = 3 \times 11.2 \, \text{km/s} = 33.6 \, \text{km/s} \] 3. **Use Conservation of Energy:** The total mechanical energy at the surface of the Earth (initial) is equal to the total mechanical energy at infinity (final). \[ \text{K.E.}_{\text{initial}} + \text{P.E.}_{\text{initial}} = \text{K.E.}_{\text{final}} + \text{P.E.}_{\text{final}} \] At the surface of the Earth: - Kinetic Energy (K.E.) = \( \frac{1}{2} m v_i^2 \) - Potential Energy (P.E.) = \( -\frac{GMm}{R} \) At infinity: - K.E. = \( \frac{1}{2} m v_{\infty}^2 \) - P.E. = 0 (since gravitational pull is negligible) 4. **Set Up the Equation:** \[ \frac{1}{2} m v_i^2 - \frac{GMm}{R} = \frac{1}{2} m v_{\infty}^2 \] 5. **Cancel Mass (m) from the Equation:** \[ \frac{1}{2} v_i^2 - \frac{GM}{R} = \frac{1}{2} v_{\infty}^2 \] 6. **Substituting Escape Velocity:** The escape velocity \( v_e \) is given by: \[ v_e = \sqrt{\frac{2GM}{R}} \] Therefore, \( \frac{GM}{R} = \frac{1}{2} v_e^2 \). 7. **Substituting Back into the Equation:** \[ \frac{1}{2} v_i^2 - \frac{1}{2} v_e^2 = \frac{1}{2} v_{\infty}^2 \] 8. **Multiply Through by 2:** \[ v_i^2 - v_e^2 = v_{\infty}^2 \] 9. **Solve for \( v_{\infty} \):** \[ v_{\infty}^2 = v_i^2 - v_e^2 \] \[ v_{\infty} = \sqrt{v_i^2 - v_e^2} \] 10. **Substituting Values:** \[ v_i = 33.6 \, \text{km/s}, \quad v_e = 11.2 \, \text{km/s} \] \[ v_{\infty} = \sqrt{(33.6)^2 - (11.2)^2} \] \[ v_{\infty} = \sqrt{1128.96 - 125.44} = \sqrt{1003.52} \approx 31.7 \, \text{km/s} \] ### Final Answer: The velocity of the body when it escapes from the gravitational pull of Earth is approximately \( 31.7 \, \text{km/s} \).

To solve the problem, we will use the principle of conservation of energy. The total mechanical energy (kinetic + potential) of the body when it is projected upwards should equal the total mechanical energy when it escapes the gravitational pull of the Earth. ### Step-by-Step Solution: 1. **Identify Given Values:** - Initial velocity of the body, \( v_i = 3 \times 11.2 \, \text{km/s} \) - Escape velocity from the surface of the Earth, \( v_e = 11.2 \, \text{km/s} \) ...
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