Newton's 3rd Law applied to binary stars

In summary, the question is about the magnitude of the gravitational force between a 50 Solar mass O-type star and a 0.1 Solar mass M-type star. The correct answer is that the force is the same, as explained by Newton's 3rd Law and the Law of Universal Gravitation. The difference in their accelerations is due to their different masses, but the force between them is always equal and opposite.
  • #1
Ki_Ryn
3
0
Below is a question I recently got wrong, and the (automated) feedback.

Consider a binary system with a 50 Solar mass O-type star and a 0.1 Solar mass M-type star, the O-type star is much, much more massive than the M-type star so the magnitude of the gravitational force on the O star from the M star is ( ? ) than the force on the M star from the O star.
Selected Answer: 500 times larger
Correct Answer: the same

Feedback: Incorrect, think Newton's 3rd Law and the Law of Universal Gravitation, which show that the forces must be equal.

Since the stars are in a stable configuration, I realize that the forces must be equal, but I thought that the differing gravitational forces were balanced by the centripetal forces of the orbit (the smaller star being less massive but moving faster to compensate). In the question, it asks specifically for the gravitational force. The big star is more massive and so will have a larger gravitational pull on the small star (and everything else in the universe).

This has always confused me. Can someone confirm that I'm wrong and help me understand why?
 
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  • #2
let m be small mass, M large mass, then the force is given by

F = [tex]\frac{G.m.M}{r^{2}}[/tex]

this will act equal and opposite on both masses (Newtons 3rd law) however the acceleration it causes will be quite different

from the 2nd law we know F = ma so a = F/a

small mass
a = F/m = [tex]\frac{G.M}{r^{2}}[/tex]

large mass
A = F/M = [tex]\frac{G.m}{r^{2}}[/tex]

so the relative accelerations differ by m/M in magnitude, and in terms of centripetal motiaon with r a ~[tex]\omega^{2}.r[/tex] so the radius of rotation will differ by a similar amount

anyway in conclusion the force between 2 bodies interacting through gravitation is always the equal & opposite on each body, the difference is in the acceleration caused, as the larger body has a much larger inertial resistance (mass) and vice versa
 
  • #3
Ki_Ryn said:
The big star is more massive and so will have a larger gravitational pull on the small star (and everything else in the universe).

This has always confused me. Can someone confirm that I'm wrong and help me understand why?

Welcome to PF.

The force is the same.

If we pull on a rope against each other and the rope is not moving then I'm pulling with the same force that you are pulling.

In the case you cite, one may have a greater centripetal acceleration ... but they didn't ask that. They asked about the gravitational force. So yes one has greater centripetal acceleration, but the force between the bodies is the same. And Newton's Law of Gravity is based on the product of the masses divided by the radius squared. That must be the same at each end.
 

FAQ: Newton's 3rd Law applied to binary stars

What is Newton's 3rd Law applied to binary stars?

Newton's 3rd Law states that for every action, there is an equal and opposite reaction. This law applies to binary stars, which are two stars that orbit around a common center of mass. The gravitational force between the stars is equal in magnitude and opposite in direction, according to this law.

How does Newton's 3rd Law affect the motion of binary stars?

The application of Newton's 3rd Law to binary stars means that the stars will orbit around each other in a stable manner, with their motions being determined by the balance of the gravitational forces between them. The more massive star will have a smaller orbit, while the less massive star will have a larger orbit.

Can Newton's 3rd Law be used to calculate the mass of binary stars?

Yes, Newton's 3rd Law can be used to calculate the mass of binary stars. By observing the orbital period and distance between the stars, the mass of each star can be determined using Newton's Law of Universal Gravitation and the knowledge that the gravitational force between the stars is equal and opposite.

How do binary stars provide evidence for the validity of Newton's 3rd Law?

Binary stars provide evidence for the validity of Newton's 3rd Law as they follow its predictions and exhibit stable orbits around a common center of mass. This consistent behavior is a testament to the accuracy and applicability of this fundamental law of physics.

Are there any exceptions to Newton's 3rd Law in binary stars?

In general, there are no exceptions to Newton's 3rd Law in binary stars. However, in some rare cases, the orbits of binary stars may be disrupted by other factors such as the presence of a third star or the effects of relativity. These exceptions do not invalidate the overall application of Newton's 3rd Law to binary stars.

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