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A satellite is launched into a circular orbit of radius 'R' around earth while a second satellite is launched into an orbit or radius 1.02 R. The percentage difference in the time periods of the two satellites is

A

0.7

B

`1.0`

C

1.5

D

`3.0`

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The correct Answer is:
To find the percentage difference in the time periods of two satellites in different circular orbits around Earth, we can follow these steps: ### Step 1: Understand the relationship between time period and radius According to Kepler's third law, the square of the time period (T) of a satellite is directly proportional to the cube of the radius (R) of its orbit. Mathematically, this can be expressed as: \[ T^2 \propto R^3 \] This implies: \[ T \propto R^{3/2} \] ### Step 2: Express the time period for both satellites Let the time period of the first satellite (radius R) be \( T_1 \) and the time period of the second satellite (radius 1.02R) be \( T_2 \). Using the proportionality, we can write: \[ T_1 = k \cdot R^{3/2} \] \[ T_2 = k \cdot (1.02R)^{3/2} \] where \( k \) is a constant. ### Step 3: Calculate \( T_2 \) Now, we can calculate \( T_2 \): \[ T_2 = k \cdot (1.02^{3/2}) \cdot R^{3/2} \] ### Step 4: Find the ratio of the time periods To find the percentage difference, we first need to find the ratio of \( T_2 \) to \( T_1 \): \[ \frac{T_2}{T_1} = \frac{k \cdot (1.02^{3/2}) \cdot R^{3/2}}{k \cdot R^{3/2}} = 1.02^{3/2} \] ### Step 5: Calculate \( 1.02^{3/2} \) Now, we can calculate \( 1.02^{3/2} \): \[ 1.02^{3/2} = (1.02^{1.5}) \approx 1.03 \] (using a calculator or approximation) ### Step 6: Find the percentage difference in time periods The percentage difference in time periods can be calculated as: \[ \text{Percentage Difference} = \left( \frac{T_2 - T_1}{T_1} \right) \times 100\% \] Substituting \( T_2 = 1.03 T_1 \): \[ \text{Percentage Difference} = \left( \frac{1.03 T_1 - T_1}{T_1} \right) \times 100\% = (0.03) \times 100\% = 3\% \] ### Final Answer The percentage difference in the time periods of the two satellites is **3%**. ---

To find the percentage difference in the time periods of two satellites in different circular orbits around Earth, we can follow these steps: ### Step 1: Understand the relationship between time period and radius According to Kepler's third law, the square of the time period (T) of a satellite is directly proportional to the cube of the radius (R) of its orbit. Mathematically, this can be expressed as: \[ T^2 \propto R^3 \] This implies: \[ T \propto R^{3/2} \] ...
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