Uniform circular motion with unknown mass

In summary, two satellites are in circular orbits around an unknown planet. The first satellite has a speed of 1.7x10^4 m/s and a radius of 5.25x10^6 meters, while the second satellite has a radius of 8.6x10^6 meters. The only force causing the satellites to be in orbit is the gravitational force of the unknown planet. By equating the centripetal force and gravitational force, you can find the orbital speed of the second satellite by using the variables from the first satellite's orbit.
  • #1
Emil Zapotec
3
0

Homework Statement


A satellite is in a circular orbit around an unknown planet. The satellite has a speed of 1.7x10^4 m/s and the radius is 5.25x10^6 meters. A second satellite also has a circular orbit around the same planet and has an orbit radius of 8.6x10^6 meters. What is the orbital speed of the second satellite?

The Attempt at a Solution


I was wondering if I have to find the centripetal acceleration of the first satellite. If so I know the acceleration is 55.05 m/s^2. But I'm stuck on what to do with there because I don't even know if that acceleration is relevance and how you work it into mv^2/r
 
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  • #2
What force is causing the satellite to be in circular orbit? Do you know any equations for this force?
 
  • #3
The only force would be the gravitational force of the unknown planet. But there's no information about the planet, only that a satellite rotates around it, so I'm assuming there's a formula that I need to derive where a mass needs to cancel?
 
  • #4
As the gravitational force is the only force, how about equating it to the centripetal force?
 
  • #5
Oh, so just find the centripetal force of the first one, find out what it is and equate it to the centripetal force of the satellite with the unknown velocity? I guess I made it a lot harder than I thought, thanks a lot.
 
  • #6
Well, the centripetal force of the first satellite isn't the same as the centripetal force on the second satellite. But, once you've equated the centripetal force and gravitational forces together, can you re-write the expression so one side of the equation has only constants, and the other side has the variables. Now, as one side has only constants, you can equate the variables of the two satellites. I guess I'm saying use proportionality, but in a really round-about way!
 

FAQ: Uniform circular motion with unknown mass

What is uniform circular motion?

Uniform circular motion is the motion of an object traveling in a circular path at a constant speed.

How is uniform circular motion different from regular circular motion?

Uniform circular motion refers to a specific type of circular motion where the speed of the object remains constant, while regular circular motion can have varying speeds.

How do you calculate the centripetal force in uniform circular motion?

The centripetal force in uniform circular motion can be calculated by multiplying the mass of the object by the square of its velocity, and then dividing by the radius of the circular path.

Can an object have uniform circular motion without a force acting on it?

No, an object cannot have uniform circular motion without a force acting on it. In order for an object to continuously move in a circular path at a constant speed, there needs to be a centripetal force acting towards the center of the circle.

How can you determine the mass of an object in uniform circular motion if the speed and radius are known?

The mass of an object in uniform circular motion can be determined by using the formula F = mv^2/r, where F is the centripetal force, m is the mass, v is the speed, and r is the radius of the circular path. Rearranging the formula to solve for mass, we get m = Fr/v^2.

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