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Neglecting air resistance, a 1.0-kg proj...

Neglecting air resistance, a 1.0-kg projectile has an escape velocity of about 11km/s at the surface of Earth. The corresponding escape velocity for a 2.0 kg projectile is:

A

3.5 km/s

B

5.5 km/s

C

7.1 km/s

D

11 km/s

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The correct Answer is:
To determine the escape velocity for a 2.0 kg projectile, we need to understand that escape velocity is independent of the mass of the projectile. Here's how we can arrive at the solution step by step: ### Step-by-Step Solution: 1. **Understand Escape Velocity**: Escape velocity is the minimum velocity required for an object to break free from the gravitational attraction of a celestial body without any additional propulsion. 2. **Formula for Escape Velocity**: The escape velocity (V₀) can be derived from the energy conservation principle. The formula for escape velocity from the surface of a planet is given by: \[ V_0 = \sqrt{\frac{2GM}{R}} \] where G is the universal gravitational constant, M is the mass of the Earth, and R is the radius of the Earth. 3. **Given Information**: The problem states that a 1.0 kg projectile has an escape velocity of about 11 km/s. This value is derived from the formula above and is constant for any object projected from the surface of the Earth, regardless of its mass. 4. **Mass Independence**: Since escape velocity does not depend on the mass of the projectile, the escape velocity for a 2.0 kg projectile will be the same as that for a 1.0 kg projectile. 5. **Conclusion**: Therefore, the escape velocity for the 2.0 kg projectile is also: \[ V_0 = 11 \text{ km/s} \] ### Final Answer: The escape velocity for a 2.0 kg projectile is **11 km/s**. ---

To determine the escape velocity for a 2.0 kg projectile, we need to understand that escape velocity is independent of the mass of the projectile. Here's how we can arrive at the solution step by step: ### Step-by-Step Solution: 1. **Understand Escape Velocity**: Escape velocity is the minimum velocity required for an object to break free from the gravitational attraction of a celestial body without any additional propulsion. 2. **Formula for Escape Velocity**: The escape velocity (V₀) can be derived from the energy conservation principle. The formula for escape velocity from the surface of a planet is given by: \[ ...
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