Calculate Geosynchronous Orbit Dist. to Earth's Center

  • Thread starter Shaunzio
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In summary, the conversation is about calculating the distance in meters from a satellite to the Earth's center in a circular, geosynchronous orbit with a period of 24 hours. The equation used is T=((2*Pi)*r^(3/2))/sqrt(GM) and the correct answer is 4.2*10^7 meters. There is also a discussion about the units of T and the need to check the units in the formula.
  • #1
Shaunzio
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Homework Statement


A satellite is in a circular, geosynchronous orbit (makes one revolution around Earth in 24 hours). Calculate the distance in meters from the satellite to the Earth's center. Mass of Earth = 5.97 x 1024 kg



Homework Equations


T=((2*Pi)*r^(3/2))/sqrt(GM)


The Attempt at a Solution



I thought T equals the period 2Pi. So the the 2Pi's cancel and then you just plug in the variables. Unfortunately I'm not getting the right answer which is supposed to be: 4.2*10^7.

Any help would be greatly appreciated.
 
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  • #2
Check to see what units the formula will produce.
 
  • #3
Would the units for T be radians?
 
  • #4
Shaunzio said:
Would the units for T be radians?
You're guessing? Why don't you expand the units from the formula and actually see what it is?
 
  • #5



Your approach is on the right track, but there are a few errors in your calculation. First, the value of T should be 24 hours, not 2Pi. This is because the period of a geosynchronous orbit is equal to the time it takes for the satellite to complete one full revolution around the Earth, which in this case is 24 hours. Second, the equation you are using is for the period of an orbit, not the distance. To calculate the distance, you will need to rearrange the equation and solve for r. The correct equation to use is r = (GMT^2 / 4π^2)^(1/3). Plugging in the values given, the distance from the satellite to the Earth's center is approximately 4.2*10^7 meters. It's important to double check your equations and make sure you are using the correct units for each variable. Keep up the good work!
 

Related to Calculate Geosynchronous Orbit Dist. to Earth's Center

1. What is a geosynchronous orbit?

A geosynchronous orbit is an orbit around the Earth that has the same orbital period as the Earth's rotation, meaning that the satellite remains in a fixed position relative to the Earth's surface. This type of orbit is commonly used for communication and weather satellites.

2. How is the distance to Earth's center calculated for a geosynchronous orbit?

The distance to Earth's center for a geosynchronous orbit is calculated using the formula: r = (G * M * T^2 / 4π^2)^(1/3), where r is the distance to Earth's center, G is the gravitational constant, M is the mass of the Earth, and T is the orbital period.

3. What is the value of the gravitational constant (G)?

The gravitational constant (G) is a physical constant that is used to calculate the force of gravity between two objects. It has a value of approximately 6.67 x 10^-11 m^3/kg*s^2.

4. How does the distance to Earth's center affect a geosynchronous orbit?

The distance to Earth's center affects a geosynchronous orbit by determining the orbital period and speed of the satellite. The closer a satellite is to Earth's center, the shorter its orbital period and the faster its orbital speed will be. This is important for maintaining a fixed position above a specific location on Earth's surface.

5. Can the distance to Earth's center for a geosynchronous orbit be changed?

Yes, the distance to Earth's center for a geosynchronous orbit can be changed by adjusting the satellite's velocity or by using thrusters to change its orbit. However, this is a complex and costly process, so satellites are typically placed in their geosynchronous orbits during launch.

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