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A body is projected vertically upwards from the surface of earth with a velocity equal to half the escape velocity. If R be the radius of earth, maximum height attained by the body from the surface of earth is `( R)/(n)`. Find the value of n.

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To solve the problem, we will use the principle of conservation of mechanical energy. The body is projected upwards with a velocity equal to half the escape velocity, and we need to find the maximum height attained by the body from the surface of the Earth. ### Step-by-Step Solution: 1. **Understanding Escape Velocity**: The escape velocity \( v_e \) from the surface of the Earth is given by the formula: \[ v_e = \sqrt{2gR} \] where \( g \) is the acceleration due to gravity at the surface of the Earth and \( R \) is the radius of the Earth. 2. **Initial Velocity**: Since the body is projected with a velocity equal to half the escape velocity, we have: \[ v = \frac{1}{2} v_e = \frac{1}{2} \sqrt{2gR} \] 3. **Initial Kinetic Energy**: The initial kinetic energy \( K_i \) of the body is given by: \[ K_i = \frac{1}{2} mv^2 = \frac{1}{2} m \left(\frac{1}{2} \sqrt{2gR}\right)^2 = \frac{1}{2} m \cdot \frac{1}{4} (2gR) = \frac{mgR}{4} \] 4. **Initial Potential Energy**: The initial potential energy \( U_i \) at the surface of the Earth is: \[ U_i = -\frac{GMm}{R} \] where \( G \) is the universal gravitational constant and \( M \) is the mass of the Earth. 5. **Final Kinetic Energy and Potential Energy**: At the maximum height \( h \), the final kinetic energy \( K_f \) is 0 (the body momentarily comes to rest), and the potential energy \( U_f \) at height \( h \) is: \[ U_f = -\frac{GMm}{R + h} \] 6. **Applying Conservation of Energy**: According to the conservation of mechanical energy: \[ K_i + U_i = K_f + U_f \] Substituting the values we have: \[ \frac{mgR}{4} - \frac{GMm}{R} = 0 - \frac{GMm}{R + h} \] 7. **Simplifying the Equation**: Rearranging gives: \[ \frac{mgR}{4} - \frac{GMm}{R} = -\frac{GMm}{R + h} \] Canceling \( m \) from both sides: \[ \frac{gR}{4} - \frac{GM}{R} = -\frac{GM}{R + h} \] 8. **Substituting \( g \)**: We know \( g = \frac{GM}{R^2} \), substituting this into the equation: \[ \frac{GM}{R^2} \cdot \frac{R}{4} - \frac{GM}{R} = -\frac{GM}{R + h} \] Simplifying gives: \[ \frac{GM}{4R} - \frac{GM}{R} = -\frac{GM}{R + h} \] \[ \frac{GM}{4R} - \frac{4GM}{4R} = -\frac{GM}{R + h} \] \[ -\frac{3GM}{4R} = -\frac{GM}{R + h} \] 9. **Cross Multiplying**: Cross multiplying gives: \[ 3G(R + h) = 4GR \] Simplifying: \[ 3R + 3h = 4R \] \[ 3h = R \] \[ h = \frac{R}{3} \] 10. **Finding \( n \)**: From the problem, we have \( h = \frac{R}{n} \). Since we found \( h = \frac{R}{3} \), we can equate: \[ \frac{R}{n} = \frac{R}{3} \] Thus, \( n = 3 \). ### Final Answer: The value of \( n \) is \( 3 \).
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