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The escape velocity from the surface of ...

The escape velocity from the surface of the earth is `V_(e)`. The escape velcotiy from the surface of a planet whose mass and radius are three times those of the earth, will be

A

`v_(e)`

B

`3v_(e)`

C

`9v_(e)`

D

`(1)/(3v_(e))`

Text Solution

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The correct Answer is:
To find the escape velocity from the surface of a planet whose mass and radius are three times those of the Earth, we can follow these steps: ### Step-by-Step Solution: 1. **Understand the formula for escape velocity**: The escape velocity (V_e) from the surface of a celestial body is given by the formula: \[ V_e = \sqrt{\frac{2GM}{R}} \] where \( G \) is the universal gravitational constant, \( M \) is the mass of the body, and \( R \) is the radius of the body. 2. **Identify the parameters for Earth**: Let the mass of the Earth be \( M_E \) and the radius of the Earth be \( R_E \). The escape velocity from the surface of the Earth is given as \( V_e \). 3. **Parameters for the new planet**: For the new planet, we are given: - Mass \( M_P = 3M_E \) (three times the mass of the Earth) - Radius \( R_P = 3R_E \) (three times the radius of the Earth) 4. **Substitute the parameters into the escape velocity formula for the new planet**: Using the escape velocity formula for the new planet: \[ V_P = \sqrt{\frac{2G \cdot M_P}{R_P}} \] Substituting \( M_P \) and \( R_P \): \[ V_P = \sqrt{\frac{2G \cdot (3M_E)}{3R_E}} \] 5. **Simplify the expression**: We can simplify the expression: \[ V_P = \sqrt{\frac{2G \cdot 3M_E}{3R_E}} = \sqrt{\frac{2GM_E}{R_E}} \] Since \( V_e = \sqrt{\frac{2GM_E}{R_E}} \) (the escape velocity from Earth), we can substitute: \[ V_P = V_e \] 6. **Conclusion**: Thus, the escape velocity from the surface of the planet is equal to the escape velocity from the surface of the Earth: \[ V_P = V_e \] ### Final Answer: The escape velocity from the surface of the planet is \( V_e \).
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Knowledge Check

  • The escape velocity from the surface of the earth is (where R_(E) is the radius of the earth )

    A
    `sqrt(2gR_(E))`
    B
    `sqrt(gR_(E))`
    C
    `2sqrt(gR_(E))`
    D
    `sqrt(3gR_(E))`
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