How Do You Calculate the Net Force on a Satellite in Circular Orbit?

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In summary, the question is about the net force of six artificial satellites completing a circular orbit around a space station in the same amount of time. Each satellite has a mass of m and radius of orbit L. The equation for the force is given as F=mv^2/L and the attempt at a solution involves finding the velocity (v) using the equation for motion in a circle. However, the time (T) is unknown and it is assumed to be 1. Another question is raised about the force of gravity between two masses and the mass of the space station.
  • #1
iluvphys
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Hello friends, I have a question considering Newton in circular motion.

Homework Statement


Six artificial satellites complete one circular orbit around a space station in the same amount of time. Each satellite has mass m and radius of orbit L.
What is the net force of every single satellite?

e.g. - S1: m= 300kg L= 7500m

If I know how to work one of them out I can do the rest.

Homework Equations



F = mv^2/L

I know m, know L but have to figure out v.



The Attempt at a Solution


Well, I started writing down the equation for motion in a circle and got Fnet=mv^2/L.
I was hoping I could replace v with 2*pi*L/T.
However I don't know T. I am assuming that since the time taken for the round trips is the same for every satellite, I could assume T being 1 couldn't I?
Please help and thanks in advance.
 
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  • #2
How about the equation for the force of gravity between two masses?

Also, what about the mass of the space station?
 
  • #3


Hello there, in response to your question, the net force acting on each satellite would be equal to the centripetal force required to keep them in circular motion. This force can be calculated using the equation F = mv^2/L, where m is the mass of the satellite, v is the velocity, and L is the radius of the orbit. Since all six satellites have the same mass and radius of orbit, the net force on each of them would be the same.

In order to calculate the velocity, we can use the formula for the period of a circular orbit, T = 2π√(L^3/GM), where G is the gravitational constant and M is the mass of the space station. Since the time taken for one orbit is the same for all satellites, we can use this equation to find the velocity for each satellite.

Therefore, the net force on each satellite would be F = m(2πL/T)^2/L, where T is the period calculated using the above equation. I hope this helps, and please let me know if you have any further questions. Good luck with your homework!
 

FAQ: How Do You Calculate the Net Force on a Satellite in Circular Orbit?

What is Newton's satellite problem?

The Newton's satellite problem is a physics problem that involves determining the motion of a satellite orbiting a celestial object, such as a planet or a star, under the influence of gravity. It was first formulated by Sir Isaac Newton in his famous book "Principia Mathematica".

What are the key factors that influence the motion of a satellite in Newton's satellite problem?

The key factors that influence the motion of a satellite in Newton's satellite problem are the mass of the satellite, the mass of the celestial object it is orbiting, and the distance between them. Other factors such as the shape of the orbit, the velocity of the satellite, and external forces also play a role.

How is Newton's satellite problem solved?

Newton's satellite problem is solved using his laws of motion and his law of universal gravitation. These laws describe the relationship between the forces acting on the satellite and its motion, allowing us to calculate the trajectory of the satellite's orbit.

What is the significance of Newton's satellite problem?

The significance of Newton's satellite problem lies in its application in modern space technology. By understanding the motion of satellites, we are able to design and launch satellites into specific orbits for various purposes such as communication, navigation, and scientific research.

Are there any real-life examples of Newton's satellite problem?

Yes, there are many real-life examples of Newton's satellite problem. Some examples include the moon orbiting around the Earth, the Earth orbiting around the sun, and artificial satellites orbiting around the Earth. These examples demonstrate the accuracy and applicability of Newton's laws of motion and gravitation.

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