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A satellite is revolving around earth in...

A satellite is revolving around earth in its equatorial plane with a period `T`. If the radius of earth suddenly shrinks to half without change in the mass. Then, the new period of revolution will be

A

`8 T`

B

`2sqrt(2) T`

C

`2T`

D

`T`

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AI Generated Solution

The correct Answer is:
To solve the problem, we need to understand how the period of a satellite in orbit is affected by the radius of the Earth. The period \( T \) of a satellite in a circular orbit is given by the formula: \[ T = 2\pi \sqrt{\frac{r^3}{GM}} \] where: - \( T \) is the orbital period, - \( r \) is the distance from the center of the Earth to the satellite, - \( G \) is the gravitational constant, - \( M \) is the mass of the Earth. ### Step-by-Step Solution: 1. **Initial Conditions**: Let the initial radius of the orbit be \( r \) (which is the radius of the Earth plus the altitude of the satellite). The period of the satellite is given as \( T \). 2. **Change in Radius**: According to the problem, the radius of the Earth shrinks to half. Therefore, the new radius \( r' \) of the orbit will be: \[ r' = \frac{r}{2} \] 3. **New Period Calculation**: We need to find the new period \( T' \) using the same formula: \[ T' = 2\pi \sqrt{\frac{(r')^3}{GM}} \] Substituting \( r' = \frac{r}{2} \): \[ T' = 2\pi \sqrt{\frac{\left(\frac{r}{2}\right)^3}{GM}} = 2\pi \sqrt{\frac{\frac{r^3}{8}}{GM}} = 2\pi \sqrt{\frac{r^3}{8GM}} \] 4. **Relating New Period to Old Period**: We know from the original period: \[ T = 2\pi \sqrt{\frac{r^3}{GM}} \] Now, we can express \( T' \) in terms of \( T \): \[ T' = 2\pi \sqrt{\frac{1}{8}} \sqrt{\frac{r^3}{GM}} = \frac{T}{\sqrt{8}} = \frac{T}{2\sqrt{2}} \] 5. **Final Answer**: Therefore, the new period of revolution when the radius of the Earth shrinks to half is: \[ T' = \frac{T}{2\sqrt{2}} \]

To solve the problem, we need to understand how the period of a satellite in orbit is affected by the radius of the Earth. The period \( T \) of a satellite in a circular orbit is given by the formula: \[ T = 2\pi \sqrt{\frac{r^3}{GM}} \] where: - \( T \) is the orbital period, ...
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