How Do Orbital Dynamics Affect Satellites with Different Masses and Distances?

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The discussion focuses on calculating the orbital periods and gravitational forces acting on three satellites with different masses and distances from a planet. The user is initially unsure whether to consider the gravitational interactions between the satellites or only the gravitational force from the planet. They apply Kepler's third law to deduce that satellite s2, with the same orbital radius as s1, would have the same period of 250 minutes. For satellite s3, they calculate its period based on the increased radius, suggesting it would be 250 multiplied by 1.5 cubed. The forces acting on satellites s2 and s3 are also derived, indicating that s2 experiences a force of 20,000 N and s3 experiences a force adjusted for its distance.
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Homework Statement


Three satellites orbit a planet of radius R. Satellites s1 and s3 have mass m. Satellite s2 has a mass of 2m. Satellites s1 & s2 have orbits 2R from the center of the planet. Satellite s3 has an orbit of 3R from the center of the planet. Satellite s1 orbits in 250 minutes and the force on s1 is 10,000 N

a)What are the periods of s2 and s3?
b)What are the forces on s2 and s3

Homework Equations


T= [(4pi)^2/GM]*r^3


The Attempt at a Solution



As I'm starting this problem, I'm wondering: Do I have to consider the forces between the satellites as well? And if I do, how will I know the distances between them? Or is the force on s1 only the force from the gravity of the planet? Can I get some suggestions on how to start this?
 
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Is this going to end up being an expression or a number?
 
Ok, I just had some thoughts, according to Kepler's third law it seems to me that satellite 2 would also have a period of 250 minutes. Then by reasoning, increasing the radius by a factor of 1.5 would increase the period by a factor of 1.5^3 so the period of s3 would be 250* (1.5)^3. Is this correct?
 
F= GMm/r^2 So Then likewise, the force on s2 would be 20,000N & s3 would be 10000/(1.5^2)
 
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