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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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a

r=GMT24π23, v=2πrT

b

r=GMT4π23, v=2πrT

c

r=GMT34π23, v=2πrT

d

r=GMT2π23, v=2πrT 

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,
Fc=MV2r The gravitational pull between two objects will then be discovered. Using the formula below,
Fc=GMmr2 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.
mv2r=GMmr2 Simplifying the equation above yields the relation shown below.
v=GMrif the orbital length is 2r and the rotational time is T. Therefore, we may write the equation below.
v=2πrTThe following equation is implied;
2πrT=GMrThis is simplified to give us the equation that follows;
r=GMT2π23We 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;
v=2πrTWe 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 r=GMT2π23 ,v=2πrT.
Hence, option 1 is correct.
 
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