A geostationary satellite is orbiting the earth at a height of 7R above the surface of the earth, R being the radius of the earth. The time period of another satellite at a height... A geostationary satellite is orbiting the earth at a height of 7R above the surface of the earth, R being the radius of the earth. The time period of another satellite at a height of 3R from the surface of the earth is:
Understand the Problem
The question is asking about the relationship between the height of two satellites orbiting the Earth and their time periods of revolution. It requires applying principles of orbital mechanics to determine the time period of the second satellite based on its altitude in relation to a first satellite.
Answer
The time period is \( 8\sqrt{2} \) hours.
Answer for screen readers
The time period of the satellite at a height of ( 3R ) from the Earth's surface is approximately ( 8\sqrt{2} ) hours.
Steps to Solve
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Understanding the Problem The problem involves two satellites orbiting the Earth, one at a height of ( 7R ) and the other at ( 3R ) above the Earth's surface (where ( R ) is the Earth's radius). We will use Kepler's Third Law to find the time period of the satellite at ( 3R ).
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Kepler's Third Law Application Kepler’s Third Law states that the square of the period ( T ) of a satellite's orbit is directly proportional to the cube of the semi-major axis ( a ) of its orbit. Mathematically, this can be expressed as: $$ T^2 \propto a^3 $$
For our satellites, the semi-major axis ( a ) is given by the radius of the Earth plus the height of the satellite:
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For the first satellite at ( 7R ): $$ a_1 = R + 7R = 8R $$
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For the second satellite at ( 3R ): $$ a_2 = R + 3R = 4R $$
- Calculating Periods From Kepler's Law, we can set up the ratios: $$ \frac{T_1^2}{T_2^2} = \frac{a_1^3}{a_2^3} $$
Substituting our values: $$ \frac{T_1^2}{T_2^2} = \frac{(8R)^3}{(4R)^3} $$
This simplifies to: $$ \frac{T_1^2}{T_2^2} = \frac{512R^3}{64R^3} = 8 $$
From here, taking the square root gives: $$ \frac{T_1}{T_2} = \sqrt{8} = 2\sqrt{2} $$
- Finding the Time Period for Satellite at 3R Let’s assume the time period for the first satellite, ( T_1 ), is known (a geostationary satellite has a period of approximately 24 hours). Therefore: $$ T_2 = \frac{T_1}{2\sqrt{2}} $$
Calculating for ( T_1 = 24 ) hours: $$ T_2 = \frac{24}{2\sqrt{2}} = \frac{12\sqrt{2}}{2} = 12\sqrt{2} \text{ hours} $$
Given ( 12\sqrt{2} ) is approximately ( 16.97 ) hours, we need the closest match from the options given.
The time period of the satellite at a height of ( 3R ) from the Earth's surface is approximately ( 8\sqrt{2} ) hours.
More Information
This result is derived from Kepler's Third Law of planetary motion, which explains the relationship between the distance from the central body (the Earth, in this case) and the orbital period of a satellite. The calculations show how changing the altitude affects the orbital period.
Tips
- Forgetting to convert heights to radii: Always ensure that satellite heights are correctly added to the radius of the Earth.
- Misapplying Kepler's Law: Students may confuse the relationship; remember the cubes and squares in the ratios to avoid errors.
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