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A spaceship is launched into a circular ...

A spaceship is launched into a circular orbit close to the Earth's surface. What additional velocity has to be imparted to the spaceship to overcome the gravitational pull?

A

`11.2 km s^(-1)`

B

`8 km s^(-1)`

C

`3.2 km s^(-1)`

D

`1.5 km s^(-1)`

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The correct Answer is:
To solve the problem of determining the additional velocity that needs to be imparted to a spaceship in a circular orbit close to the Earth's surface to overcome gravitational pull, we can follow these steps: ### Step-by-Step Solution: 1. **Understand the Concepts**: - **Orbital Velocity (v_o)**: The velocity required for an object to maintain a stable orbit around a planet. For a circular orbit close to the Earth's surface, the formula is: \[ v_o = \sqrt{\frac{GM}{R}} \] - **Escape Velocity (v_e)**: The minimum velocity needed for an object to break free from the gravitational attraction of a planet. The formula for escape velocity is: \[ v_e = \sqrt{\frac{2GM}{R}} \] - Here, \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( R \) is the radius of the Earth. 2. **Calculate the Additional Velocity**: - The additional velocity (\( v_{add} \)) required to overcome gravitational pull can be found by subtracting the orbital velocity from the escape velocity: \[ v_{add} = v_e - v_o \] 3. **Substituting the Formulas**: - Substitute the formulas for \( v_e \) and \( v_o \): \[ v_{add} = \sqrt{\frac{2GM}{R}} - \sqrt{\frac{GM}{R}} \] 4. **Factor Out Common Terms**: - Factor out \( \sqrt{\frac{GM}{R}} \): \[ v_{add} = \sqrt{\frac{GM}{R}} \left( \sqrt{2} - 1 \right) \] 5. **Express in Terms of Gravitational Acceleration**: - Since \( g = \frac{GM}{R} \), we can express the additional velocity as: \[ v_{add} = \sqrt{gR} \left( \sqrt{2} - 1 \right) \] 6. **Final Expression**: - Therefore, the additional velocity that needs to be imparted to the spaceship to overcome the gravitational pull is: \[ v_{add} = gR \left( \sqrt{2} - 1 \right) \] ### Final Answer: The additional velocity required to overcome the gravitational pull is \( gR \left( \sqrt{2} - 1 \right) \).
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