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In the previous problem, the minimum spe...

In the previous problem, the minimum speed with which the body must be thrown from the surface of the earth so as to reach a height of `R//4` is

A

`sqrt((gR)/2)`

B

`sqrt(gR)`

C

`sqrt((gR)/5)`

D

`sqrt((2gR)/5)`

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To solve the problem of finding the minimum speed with which a body must be thrown from the surface of the Earth to reach a height of \( \frac{R}{4} \), we can use the principle of conservation of mechanical energy. Here’s a step-by-step solution: ### Step 1: Understand the Energy Conservation Principle When the body is thrown upwards, its mechanical energy (kinetic + potential) at the surface of the Earth will be equal to its mechanical energy at the height \( \frac{R}{4} \). At the maximum height, the kinetic energy will be zero, and only potential energy will be present. ### Step 2: Write the Expression for Mechanical Energy at Two Points 1. **At the surface (Point 1)**: - Kinetic Energy (KE) = \( \frac{1}{2} mv^2 \) - Potential Energy (PE) = \( -\frac{GMm}{R} \) (where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( R \) is the radius of the Earth) Total Energy at Point 1: \[ E_1 = \frac{1}{2} mv^2 - \frac{GMm}{R} \] 2. **At the height \( \frac{R}{4} \) (Point 2)**: - Kinetic Energy (KE) = 0 (at maximum height) - Potential Energy (PE) = \( -\frac{GMm}{\frac{5R}{4}} = -\frac{4GMm}{5R} \) Total Energy at Point 2: \[ E_2 = 0 - \frac{4GMm}{5R} = -\frac{4GMm}{5R} \] ### Step 3: Set the Energies Equal According to the conservation of mechanical energy: \[ E_1 = E_2 \] Substituting the expressions we derived: \[ \frac{1}{2} mv^2 - \frac{GMm}{R} = -\frac{4GMm}{5R} \] ### Step 4: Simplify the Equation 1. Cancel \( m \) from both sides (assuming \( m \neq 0 \)): \[ \frac{1}{2} v^2 - \frac{GM}{R} = -\frac{4GM}{5R} \] 2. Rearranging gives: \[ \frac{1}{2} v^2 = \frac{GM}{R} - \frac{4GM}{5R} \] 3. Combine the terms on the right: \[ \frac{1}{2} v^2 = \frac{5GM}{5R} - \frac{4GM}{5R} = \frac{1GM}{5R} \] ### Step 5: Solve for \( v^2 \) Multiply both sides by 2: \[ v^2 = \frac{2GM}{5R} \] ### Step 6: Take the Square Root \[ v = \sqrt{\frac{2GM}{5R}} \] ### Step 7: Substitute \( g \) Using the relation \( g = \frac{GM}{R^2} \), we can express \( GM \) as \( gR \): \[ v = \sqrt{\frac{2gR}{5}} \] ### Final Result Thus, the minimum speed with which the body must be thrown from the surface of the Earth to reach a height of \( \frac{R}{4} \) is: \[ v = \sqrt{\frac{2gR}{5}} \]

To solve the problem of finding the minimum speed with which a body must be thrown from the surface of the Earth to reach a height of \( \frac{R}{4} \), we can use the principle of conservation of mechanical energy. Here’s a step-by-step solution: ### Step 1: Understand the Energy Conservation Principle When the body is thrown upwards, its mechanical energy (kinetic + potential) at the surface of the Earth will be equal to its mechanical energy at the height \( \frac{R}{4} \). At the maximum height, the kinetic energy will be zero, and only potential energy will be present. ### Step 2: Write the Expression for Mechanical Energy at Two Points 1. **At the surface (Point 1)**: - Kinetic Energy (KE) = \( \frac{1}{2} mv^2 \) ...
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