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Q.
How do you calculate the altitude and velocity of a satellite in a geosynchronous orbit of mars:
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answer is A.
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Detailed Solution
Concept: Geosynchronous orbit: A high earth orbit that enables satellites to coincide with the earth's rotation is known as a geosynchronous orbit. This orbit is 35,786 kilometres above the equator of the planet.
The procedures below must be taken in order to determine any planet's geosynchronous orbit:
To begin with, we need to understand the centripetal force acting on the item as it is rotating. Using the formula below,
The gravitational pull between two objects will then be discovered. Using the formula below,
Where r is the distance between them and M is the mass of the satellite and M is the mass of Mars.
G stands for gravity constant.
The centripetal force and gravitational force must now be equal for the satellite to remain stable in its orbit.
Simplifying the equation above yields the relation shown below.
if the orbital length is 2r and the rotational time is T. Therefore, we may write the equation below.
The following equation is implied;
This is simplified to give us the equation that follows;
We may determine the distance using the aforementioned relation. The distance to Mars' centre is shown by this measurement. We shall deduct the radius of mass from r to determine height.
We will use the following formula to determine the velocity;
We may determine the satellite's velocity in Mars' geosynchronous orbit by applying the formula above.
In light of the foregoing reasoning, it is evident how to determine a satellite's height and speed when it is in a geosynchronous orbit around Mars.
So, the correct answer is .
Hence, option 1 is correct.
The procedures below must be taken in order to determine any planet's geosynchronous orbit:
To begin with, we need to understand the centripetal force acting on the item as it is rotating. Using the formula below,
The gravitational pull between two objects will then be discovered. Using the formula below,
Where r is the distance between them and M is the mass of the satellite and M is the mass of Mars.
G stands for gravity constant.
The centripetal force and gravitational force must now be equal for the satellite to remain stable in its orbit.
Simplifying the equation above yields the relation shown below.
if the orbital length is 2r and the rotational time is T. Therefore, we may write the equation below.
The following equation is implied;
This is simplified to give us the equation that follows;
We may determine the distance using the aforementioned relation. The distance to Mars' centre is shown by this measurement. We shall deduct the radius of mass from r to determine height.
We will use the following formula to determine the velocity;
We may determine the satellite's velocity in Mars' geosynchronous orbit by applying the formula above.
In light of the foregoing reasoning, it is evident how to determine a satellite's height and speed when it is in a geosynchronous orbit around Mars.
So, the correct answer is .
Hence, option 1 is correct.
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