Satellites in orbit such that they look like they don't move

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    Orbit Satellites
AI Thread Summary
Communication satellites in geosynchronous orbit maintain a fixed position above the Earth's equator, requiring a specific angular speed and orbital radius. The angular speed can be derived using the equation w = √(GM/r), but determining the radius is essential for solving the problem. The period of revolution, T, relates to angular speed through the formula ω = 2π/T, which can help find the radius if T is known. Additional equations or information may be necessary to fully resolve the radius and angular speed. Understanding these relationships is crucial for calculating the parameters of a geosynchronous satellite's orbit.
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Homework Statement


Some communication satellites are put into a circular geosynchronius orbit in which the satellite remains above a certain postion on the Earth's equator as it orbits. Such a satellite would always be in the same position in the sky as seen from the transmitting or recieveing equipment of a communications broadcasting network. Find the angular speed of the satellites orbit necessary for it to reamin above the same point above the equator. What must be the orbitial radius of such a satellite?



Homework Equations


(GMm)\r^2=mw^2r
F=(GMm)\r^2


The Attempt at a Solution


I solved for w=squareroot(GM\r)
How am i to know what the radius is? I think i need another equation to input for the radius to find w. Then I can find the radius. Is this the right way to go?
 
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Another equation might be useful. Is there any information in the problem you haven't used? Is there any extra information you can extract from what you have used?
 
Your solution equation needs a rework.

What would the period of revolution, T, of such satellite be?

\omega = \frac{2 \pi}{T}
 
but i don't know what the radius is
 
If you've got the period of revolution, T, you can calculate the angular speed with the formula in my previous post. The satellite completes 2 \pi radians (one revolution) during this time.
 
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