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A projectile is fired vertically upwards...

A projectile is fired vertically upwards from the surface of the earth with a velocity `Kv_(e)`, where `v_(e)` is the escape velocity and `Klt1`.If `R` is the radius of the earth, the maximum height to which it will rise measured from the centre of the earth will be (neglect air resistance)

A

`R/(K^(2)-1)`

B

`R/(1-K^(2))`

C

`R(1-K^(2))`

D

`R/(1+K^(2))`

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The correct Answer is:
To solve the problem of finding the maximum height to which a projectile will rise when fired vertically upwards with a velocity \( Kv_e \) (where \( v_e \) is the escape velocity and \( K < 1 \)), we can use the principle of conservation of mechanical energy. Here’s a step-by-step solution: ### Step 1: Understand the Initial Conditions The projectile is fired with an initial velocity \( v_0 = Kv_e \). The escape velocity \( v_e \) is given by the formula: \[ v_e = \sqrt{\frac{2GM}{R}} \] where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( R \) is the radius of the Earth. ### Step 2: Calculate Initial Kinetic Energy and Potential Energy At the surface of the Earth, the initial kinetic energy \( KE_i \) and potential energy \( PE_i \) are: \[ KE_i = \frac{1}{2} m (Kv_e)^2 = \frac{1}{2} m K^2 v_e^2 \] Substituting \( v_e^2 \): \[ KE_i = \frac{1}{2} m K^2 \left(\frac{2GM}{R}\right) = \frac{m K^2 GM}{R} \] The potential energy at the surface \( PE_i \) is: \[ PE_i = -\frac{GMm}{R} \] ### Step 3: Total Mechanical Energy at the Surface The total mechanical energy \( E_i \) at the surface is: \[ E_i = KE_i + PE_i = \frac{m K^2 GM}{R} - \frac{GMm}{R} = \frac{GMm}{R} (K^2 - 1) \] ### Step 4: Energy at Maximum Height At the maximum height \( H \), the kinetic energy \( KE_f \) will be zero, and the potential energy \( PE_f \) is given by: \[ PE_f = -\frac{GMm}{H} \] The total mechanical energy at maximum height \( E_f \) is: \[ E_f = KE_f + PE_f = 0 - \frac{GMm}{H} = -\frac{GMm}{H} \] ### Step 5: Apply Conservation of Energy According to the conservation of mechanical energy: \[ E_i = E_f \] Substituting the expressions for \( E_i \) and \( E_f \): \[ \frac{GMm}{R} (K^2 - 1) = -\frac{GMm}{H} \] ### Step 6: Rearranging the Equation Cancelling \( GMm \) from both sides (assuming \( m \neq 0 \)): \[ \frac{K^2 - 1}{R} = -\frac{1}{H} \] Rearranging gives: \[ \frac{1}{H} = \frac{1 - K^2}{R} \] Thus, \[ H = \frac{R}{1 - K^2} \] ### Conclusion The maximum height \( H \) to which the projectile will rise, measured from the center of the Earth, is: \[ H = \frac{R}{1 - K^2} \]

To solve the problem of finding the maximum height to which a projectile will rise when fired vertically upwards with a velocity \( Kv_e \) (where \( v_e \) is the escape velocity and \( K < 1 \)), we can use the principle of conservation of mechanical energy. Here’s a step-by-step solution: ### Step 1: Understand the Initial Conditions The projectile is fired with an initial velocity \( v_0 = Kv_e \). The escape velocity \( v_e \) is given by the formula: \[ v_e = \sqrt{\frac{2GM}{R}} \] where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( R \) is the radius of the Earth. ...
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