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Two satellites A and B of the same mass ...

Two satellites `A` and `B` of the same mass are revolving around the earth in the concentric circular orbits such that the distance of satellite `B` from the centre of the earth is thrice as compared to the distance of the satellite `A` from the centre of the earth. The ratio of the centripetal force acting on `B` as compared to that on `A` is

A

`1/3`

B

`3`

C

`1/9`

D

`1/(sqrt(3))`

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The correct Answer is:
To find the ratio of the centripetal force acting on satellite B compared to that on satellite A, we can follow these steps: ### Step 1: Define the variables Let: - \( m \) = mass of satellite A = mass of satellite B (since they are the same) - \( R_A \) = distance of satellite A from the center of the Earth - \( R_B \) = distance of satellite B from the center of the Earth According to the problem, \( R_B = 3 R_A \). ### Step 2: Write the expression for gravitational force The gravitational force \( F \) acting on a satellite in orbit is given by the formula: \[ F = \frac{G \cdot M \cdot m}{R^2} \] where: - \( G \) = universal gravitational constant - \( M \) = mass of the Earth - \( m \) = mass of the satellite - \( R \) = distance from the center of the Earth to the satellite ### Step 3: Calculate the gravitational force for both satellites For satellite A: \[ F_A = \frac{G \cdot M \cdot m}{R_A^2} \] For satellite B: \[ F_B = \frac{G \cdot M \cdot m}{R_B^2} \] ### Step 4: Substitute \( R_B \) in terms of \( R_A \) Since \( R_B = 3 R_A \), we can substitute this into the equation for \( F_B \): \[ F_B = \frac{G \cdot M \cdot m}{(3 R_A)^2} = \frac{G \cdot M \cdot m}{9 R_A^2} \] ### Step 5: Find the ratio of the forces Now, we can find the ratio of the centripetal forces (which are equal to the gravitational forces) acting on satellites B and A: \[ \frac{F_B}{F_A} = \frac{\frac{G \cdot M \cdot m}{9 R_A^2}}{\frac{G \cdot M \cdot m}{R_A^2}} = \frac{1}{9} \] ### Conclusion Thus, the ratio of the centripetal force acting on satellite B compared to that on satellite A is: \[ \frac{F_B}{F_A} = \frac{1}{9} \] ### Final Answer The final answer is \( \frac{1}{9} \). ---

To find the ratio of the centripetal force acting on satellite B compared to that on satellite A, we can follow these steps: ### Step 1: Define the variables Let: - \( m \) = mass of satellite A = mass of satellite B (since they are the same) - \( R_A \) = distance of satellite A from the center of the Earth - \( R_B \) = distance of satellite B from the center of the Earth ...
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