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A particle is throws vertically upwards ...

A particle is throws vertically upwards from the surface of earth and it reaches to a maximum height equal to the radius of earth. The radio of the velocity of projection to the escape velocity on the surface of earth is

A

`(1)/(sqrt2)`

B

`(1)/(2)`

C

`(1)/(4)`

D

`(1)/(2sqrt2)`

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The correct Answer is:
To solve the problem, we will use the principle of conservation of energy. We need to find the ratio of the velocity of projection (V₁) to the escape velocity (Vₑ) on the surface of the Earth. ### Step-by-Step Solution: 1. **Understand the Problem**: A particle is thrown vertically upwards and reaches a maximum height equal to the radius of the Earth (R). We need to find the ratio of the initial velocity of projection (V₁) to the escape velocity (Vₑ). 2. **Define Escape Velocity**: The escape velocity (Vₑ) from the surface of the Earth is given by the formula: \[ Vₑ = \sqrt{\frac{2GM}{R}} \] where G is the gravitational constant and M is the mass of the Earth. 3. **Initial Energy (Eᵢ)**: The initial energy of the particle when it is thrown is the sum of its kinetic energy and gravitational potential energy: \[ Eᵢ = \frac{1}{2} m V₁^2 - \frac{GMm}{R} \] Here, \( m \) is the mass of the particle. 4. **Final Energy (E_f)**: At the maximum height (h = R), the kinetic energy becomes zero, and the potential energy at that height is: \[ E_f = -\frac{GMm}{2R} \] (since the height is equal to the radius of the Earth). 5. **Apply Conservation of Energy**: According to the conservation of energy, the initial energy equals the final energy: \[ Eᵢ = E_f \] Substituting the expressions we have: \[ \frac{1}{2} m V₁^2 - \frac{GMm}{R} = -\frac{GMm}{2R} \] 6. **Simplify the Equation**: Rearranging the equation gives: \[ \frac{1}{2} m V₁^2 = \frac{GMm}{R} - \frac{GMm}{2R} \] \[ \frac{1}{2} m V₁^2 = \frac{GMm}{2R} \] Dividing both sides by \( m \) (mass of the particle): \[ \frac{1}{2} V₁^2 = \frac{GM}{2R} \] Multiplying by 2: \[ V₁^2 = \frac{GM}{R} \] 7. **Calculate V₁**: Taking the square root gives: \[ V₁ = \sqrt{\frac{GM}{R}} \] 8. **Calculate the Ratio**: Now, we can find the ratio of V₁ to Vₑ: \[ \text{Ratio} = \frac{V₁}{Vₑ} = \frac{\sqrt{\frac{GM}{R}}}{\sqrt{\frac{2GM}{R}}} \] Simplifying this gives: \[ \text{Ratio} = \frac{1}{\sqrt{2}} \] 9. **Final Answer**: Therefore, the ratio of the velocity of projection to the escape velocity is: \[ \frac{V₁}{Vₑ} = \frac{1}{\sqrt{2}} \]

To solve the problem, we will use the principle of conservation of energy. We need to find the ratio of the velocity of projection (V₁) to the escape velocity (Vₑ) on the surface of the Earth. ### Step-by-Step Solution: 1. **Understand the Problem**: A particle is thrown vertically upwards and reaches a maximum height equal to the radius of the Earth (R). We need to find the ratio of the initial velocity of projection (V₁) to the escape velocity (Vₑ). 2. **Define Escape Velocity**: ...
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