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A body is projected vertically upwards f...

A body is projected vertically upwards from the surface of a planet of radius R with a velocity equal to 1/3rd the escape velocity for the planet. The maximum height attained by the body is

A

`R//2`

B

`R//3`

C

`R//5`

D

`R//9`

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The correct Answer is:
To solve the problem, we need to find the maximum height attained by a body projected vertically upwards from the surface of a planet with a velocity equal to one-third of the escape velocity. ### Step-by-Step Solution: 1. **Understand the Escape Velocity**: The escape velocity \( v_e \) from the surface of a planet is given by the formula: \[ v_e = \sqrt{2gR} \] where \( g \) is the acceleration due to gravity at the surface of the planet and \( R \) is the radius of the planet. 2. **Determine the Initial Velocity**: According to the problem, the body is projected with a velocity equal to one-third of the escape velocity: \[ u = \frac{1}{3} v_e = \frac{1}{3} \sqrt{2gR} \] 3. **Use the Equation of Motion**: The maximum height \( h \) can be found using the kinematic equation: \[ v^2 = u^2 + 2(-g)h \] At the maximum height, the final velocity \( v \) becomes 0. Thus, the equation simplifies to: \[ 0 = u^2 - 2gh \] Rearranging gives: \[ u^2 = 2gh \] 4. **Substituting the Initial Velocity**: Substitute the expression for \( u \) into the equation: \[ \left(\frac{1}{3} \sqrt{2gR}\right)^2 = 2gh \] Simplifying the left side: \[ \frac{1}{9} (2gR) = 2gh \] This leads to: \[ \frac{2gR}{9} = 2gh \] 5. **Solve for Maximum Height \( h \)**: Dividing both sides by \( 2g \): \[ \frac{R}{9} = h \] Therefore, the maximum height attained by the body is: \[ h = \frac{R}{9} \] ### Final Answer: The maximum height attained by the body is \( \frac{R}{9} \). ---

To solve the problem, we need to find the maximum height attained by a body projected vertically upwards from the surface of a planet with a velocity equal to one-third of the escape velocity. ### Step-by-Step Solution: 1. **Understand the Escape Velocity**: The escape velocity \( v_e \) from the surface of a planet is given by the formula: \[ v_e = \sqrt{2gR} ...
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DC PANDEY ENGLISH-GRAVITATION-Check Point 10.5
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