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The maximum and minimum distance of a co...

The maximum and minimum distance of a comet form the sun are `8xx10^(12)m and 1.6xx10^(12)m`. If its velocity when nearest to the sun is `60m//s`, what will be its velocity in m/s when it is farthest

A

`12`

B

`60`

C

`112`

D

`6`

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The correct Answer is:
To solve the problem, we can use the principle of conservation of angular momentum. The angular momentum of a comet about the sun remains constant as it moves in its elliptical orbit. ### Step-by-Step Solution: 1. **Identify the distances and velocities:** - Minimum distance (perihelion) from the sun, \( r_1 = 1.6 \times 10^{12} \, \text{m} \) - Maximum distance (aphelion) from the sun, \( r_2 = 8.0 \times 10^{12} \, \text{m} \) - Velocity at perihelion, \( v_1 = 60 \, \text{m/s} \) 2. **Use the conservation of angular momentum:** The angular momentum \( L \) at perihelion and aphelion can be expressed as: \[ L = m \cdot v_1 \cdot r_1 = m \cdot v_2 \cdot r_2 \] where \( m \) is the mass of the comet, \( v_2 \) is the velocity at aphelion, and \( r_2 \) is the distance at aphelion. 3. **Since the mass \( m \) is constant, we can cancel it out:** \[ v_1 \cdot r_1 = v_2 \cdot r_2 \] 4. **Rearranging the equation to find \( v_2 \):** \[ v_2 = \frac{v_1 \cdot r_1}{r_2} \] 5. **Substituting the known values:** \[ v_2 = \frac{60 \, \text{m/s} \cdot (1.6 \times 10^{12} \, \text{m})}{8.0 \times 10^{12} \, \text{m}} \] 6. **Calculating \( v_2 \):** \[ v_2 = \frac{60 \cdot 1.6}{8.0} \, \text{m/s} \] \[ v_2 = \frac{96}{8} \, \text{m/s} = 12 \, \text{m/s} \] ### Final Answer: The velocity of the comet when it is farthest from the sun is \( 12 \, \text{m/s} \).

To solve the problem, we can use the principle of conservation of angular momentum. The angular momentum of a comet about the sun remains constant as it moves in its elliptical orbit. ### Step-by-Step Solution: 1. **Identify the distances and velocities:** - Minimum distance (perihelion) from the sun, \( r_1 = 1.6 \times 10^{12} \, \text{m} \) - Maximum distance (aphelion) from the sun, \( r_2 = 8.0 \times 10^{12} \, \text{m} \) - Velocity at perihelion, \( v_1 = 60 \, \text{m/s} \) ...
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