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A satellite which is geostationary in a ...

A satellite which is geostationary in a particular orbit is taken to another orbit. Its distance from the centre of earth in new orbit is 2 times that of the earlier orbit. The time period in the second orbit is

A

(a)24 h

B

(b)48 h

C

(c)`48 sqrt(2)h`

D

(d)`48/sqrt2h`

Text Solution

AI Generated Solution

The correct Answer is:
To find the time period of a satellite in a new orbit that is twice the distance from the center of the Earth compared to its original geostationary orbit, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding the Time Period Formula**: The time period \( T \) of a satellite in orbit is given by the formula: \[ T = 2\pi \sqrt{\frac{r^3}{GM}} \] where: - \( T \) = time period of the satellite - \( r \) = distance from the center of the Earth (radius of the orbit) - \( G \) = gravitational constant - \( M \) = mass of the Earth 2. **Geostationary Orbit**: For a geostationary satellite, the time period \( T_1 \) is 24 hours (or 86400 seconds). The radius \( r_1 \) of the geostationary orbit can be calculated using the formula: \[ T_1 = 2\pi \sqrt{\frac{r_1^3}{GM}} \] 3. **New Orbit Radius**: The problem states that the new orbit's distance from the center of the Earth is twice that of the original orbit. Therefore, we have: \[ r_2 = 2r_1 \] 4. **Finding the Time Period in the New Orbit**: We can express the time period \( T_2 \) for the new orbit using the same formula: \[ T_2 = 2\pi \sqrt{\frac{r_2^3}{GM}} = 2\pi \sqrt{\frac{(2r_1)^3}{GM}} = 2\pi \sqrt{\frac{8r_1^3}{GM}} = 2\pi \sqrt{8} \sqrt{\frac{r_1^3}{GM}} \] This simplifies to: \[ T_2 = 2\pi \cdot 2\sqrt{2} \sqrt{\frac{r_1^3}{GM}} = 2\sqrt{2} T_1 \] 5. **Substituting the Time Period of the Original Orbit**: Since \( T_1 = 24 \) hours, we substitute this value: \[ T_2 = 2\sqrt{2} \cdot 24 \text{ hours} \] To calculate \( T_2 \): \[ T_2 = 48\sqrt{2} \text{ hours} \] 6. **Final Calculation**: The approximate value of \( \sqrt{2} \) is about 1.414, so: \[ T_2 \approx 48 \cdot 1.414 \approx 67.99 \text{ hours} \] ### Conclusion: The time period in the second orbit is approximately \( 67.99 \) hours.
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