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Two satellites are moving at heights of ...

Two satellites are moving at heights of R and 5R above the surface of the earth of radius R. The ratio of their velocitirs `((V_(1))/(V_(2)))` is

A

`sqrt(5):1`

B

`1 : 1`

C

`sqrt(3) : sqrt(2)`

D

`sqrt(3) : 1`

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The correct Answer is:
To solve the problem of finding the ratio of the velocities of two satellites moving at heights of R and 5R above the surface of the Earth (with Earth's radius being R), we can follow these steps: ### Step 1: Identify the distances from the center of the Earth - The radius of the Earth (R) is given. - For the first satellite (height = R above the surface), the distance from the center of the Earth is: \[ R_1 = R + R = 2R \] - For the second satellite (height = 5R above the surface), the distance from the center of the Earth is: \[ R_2 = R + 5R = 6R \] ### Step 2: Write the formula for orbital velocity The orbital velocity \( V \) of a satellite is given by the formula: \[ V = \sqrt{\frac{GM}{R}} \] where \( G \) is the gravitational constant and \( M \) is the mass of the Earth. ### Step 3: Calculate the velocities of the satellites - For the first satellite (at distance \( R_1 = 2R \)): \[ V_1 = \sqrt{\frac{GM}{R_1}} = \sqrt{\frac{GM}{2R}} \] - For the second satellite (at distance \( R_2 = 6R \)): \[ V_2 = \sqrt{\frac{GM}{R_2}} = \sqrt{\frac{GM}{6R}} \] ### Step 4: Find the ratio of the velocities To find the ratio \( \frac{V_1}{V_2} \): \[ \frac{V_1}{V_2} = \frac{\sqrt{\frac{GM}{2R}}}{\sqrt{\frac{GM}{6R}}} \] This simplifies to: \[ \frac{V_1}{V_2} = \sqrt{\frac{6R}{2R}} = \sqrt{\frac{6}{2}} = \sqrt{3} \] ### Final Answer Thus, the ratio of the velocities of the two satellites is: \[ \frac{V_1}{V_2} = \sqrt{3} \]

To solve the problem of finding the ratio of the velocities of two satellites moving at heights of R and 5R above the surface of the Earth (with Earth's radius being R), we can follow these steps: ### Step 1: Identify the distances from the center of the Earth - The radius of the Earth (R) is given. - For the first satellite (height = R above the surface), the distance from the center of the Earth is: \[ R_1 = R + R = 2R \] ...
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