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Radius of orbit of a satellite is R and T is time period. Find T' when orbit radius increase to 9R

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To solve the problem of finding the new time period \( T' \) when the radius of the satellite's orbit increases from \( R \) to \( 9R \), we can use Kepler's Third Law of planetary motion, which states that the square of the period of orbit \( T \) is directly proportional to the cube of the semi-major axis (orbital radius) of the orbit. ### Step-by-Step Solution: 1. **Understand Kepler's Third Law**: According to Kepler's Third Law, the relationship can be expressed as: \[ T^2 \propto R^3 \] This means: \[ \frac{T_1^2}{T_2^2} = \frac{R_1^3}{R_2^3} \] where \( T_1 \) and \( R_1 \) are the initial period and radius, and \( T_2 \) and \( R_2 \) are the new period and radius. 2. **Assign Values**: Let: - Initial radius \( R_1 = R \) - New radius \( R_2 = 9R \) - Initial period \( T_1 = T \) - New period \( T_2 = T' \) 3. **Set Up the Equation**: Substitute the known values into the equation: \[ \frac{T^2}{T'^2} = \frac{R^3}{(9R)^3} \] 4. **Simplify the Right Side**: Calculate \( (9R)^3 \): \[ (9R)^3 = 729R^3 \] Thus, the equation becomes: \[ \frac{T^2}{T'^2} = \frac{R^3}{729R^3} = \frac{1}{729} \] 5. **Cross Multiply**: Rearranging gives: \[ T'^2 = 729T^2 \] 6. **Take the Square Root**: To find \( T' \), take the square root of both sides: \[ T' = \sqrt{729}T = 27T \] ### Final Answer: The new time period \( T' \) when the orbit radius increases to \( 9R \) is: \[ T' = 27T \]
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