Need help with satellites and Kepler's Laws

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A user is trying to solve a problem involving a satellite's orbit around a planet of unknown mass, given its period and gravitational acceleration on the planet's surface. They initially express confusion about how to find the planet's mass and radius without direct values. Suggestions are made to use gravitational and centripetal force equations, along with Kepler's laws, to derive the necessary values. Ultimately, the user successfully figures out the solution by applying the formula for gravitational acceleration and the relationship between mass and radius. The discussion highlights the importance of understanding the relationships between orbital mechanics and gravitational forces.
fiestytig
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Here's my problem:

A 23.0-kg satellite has a circular orbit with a period of 2.35 h and a radius of 8.90×106 m around a planet of unknown mass. If the magnitude of the gravitational acceleration on the surface of the planet is 8.90 m/s2, what is the radius of the planet?

I got to say, I have no idea where to start since I don't have the mass of the planet. Any help? Pretty please? Due tonight at 10 pm EST... thanks!
 
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The force acting on the satellite is also the centripital force. F-mv^2/R and F-G(M*m)/r^2. that should help you find the mass of the planet. right?
 
First question: Do you know how to find the period of a satellite if you know the planet's mass and the Radius of its orbit?

Second question: If you do, can't you use this method to find the Planet's mass when you know the period and radius of the orbit?
 
I'm afraid I still don't follow, even with those suggestions... All I really know is T^2=4 Pi^2 r^3 /G M. But I don't really have the r either, do I?
 
fiestytig said:
I'm afraid I still don't follow, even with those suggestions... All I really know is T^2=4 Pi^2 r^3 /G M. But I don't really have the r either, do I?

Then what is this?

A 23.0-kg satellite has a circular orbit with a period of 2.35 h and a radius of 8.90×106 m around a planet of unknown mass.
 
So then how do I find the radius of the planet? (I got confused by the radiuses there for a minute.)
 
Aha! I figured it out! Thanks. Had to use a formula to find mass and then use g = G+M/R^2 to find R. :)
 
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