Is Gravitational Attraction Negligible in Oscillating Systems?

In summary: DOk, so from Kepler's third law,$$T^2=\frac{4\pi^2}{GM_{total}}a^3$$##a=\frac{L_0}{2\sqrt{2}}##$$T=\sqrt{\frac{2\pi^2}{GM_{total}}}\left(\frac{L_0}{2\sqrt{2}}\right)^{3/2}$$$$T=\frac{\pi}{\sqrt{2GM_{total}}}\cdot L_0^{3/2}$$Hence, the time period of oscillation is$$T=\frac{\pi}{\sqrt{2
  • #36
ehild said:
The area is correct. Show details of getting ωf. The formula for vpf in #11 was still correct.

ehild

I had $$v_{pf}^2=\frac{kq^2(3\sqrt{2}-4)}{10mL_0} \Rightarrow \omega_f^2L_0^2/2=\frac{kq^2(3\sqrt{2}-4)}{10mL_0}$$
It is given in the question that ##kq^2/(mL_0^3)=10^4 s^{-2}##, plugging this, I reached the value of ##\omega_f##.
 
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  • #37
Pranav-Arora said:
I had $$v_{pf}^2=\frac{kq^2(3\sqrt{2}-4)}{10mL_0} \Rightarrow \omega_f^2L_0^2/2=\frac{kq^2(3\sqrt{2}-4)}{10mL_0}$$
It is given in the question that ##kq^2/(mL_0^3)=10^4 s^{-2}##, plugging this, I reached the value of ##\omega_f##.

That is correct. What is then rf2ωf?

ehild
 
  • #38
ehild said:
That is correct. What is then rf2ωf?

ehild

I guess I made a mistake in my previous post. ##r_f=L_0/\sqrt{2}##, correct?

This time I get,
[tex]\frac{L_0^2}{2}\sqrt{2\times 10^3 (3\sqrt{2}-4)}=\frac{2\pi}{P}\frac{5L_0^2}{32}[/tex]
Solving for P, ##P=0.0891 sec##. Can you please check my post #28 and see if I used the right values for ##a## and ##b##?
 
  • #39
What did you get using Kepler's 3rd law?
 
  • #40
WannabeNewton said:
What did you get using Kepler's 3rd law?

I couldn't apply that to this problem so I continued with the second law. :uhh:
 
  • #41
Pranav-Arora said:
I guess I made a mistake in my previous post. ##r_f=L_0/\sqrt{2}##, correct?

This time I get,
[tex]\frac{L_0^2}{2}\sqrt{2\times 10^3 (3\sqrt{2}-4)}=\frac{2\pi}{P}\frac{5L_0^2}{32}[/tex]
Solving for P, ##P=0.0891 sec##. Can you please check my post #28 and see if I used the right values for ##a## and ##b##?

That looks correct.

ehild
 
  • #43
Here's a video of the motion:

[I will delete this post if animations are not allowed to be uploaded or if it doesn't work for some reason. File size is 191.3 KB]
 

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  • #44
Oh my god TSny I've been spending the last hour trying to make an animation of the system motion; you are absolutely brilliant I love you :)! You're going to have to tell me what program you used to make that.
 
  • #45
WannabeNewton said:
You're going to have to tell me what program you used to make that.

I used Mathematica. I searched the net today to find out how to export a Mathematica animation. I'm not an experienced programmer. Glad that it seems to be working.
 
  • #46
Yeah it works great! Thanks. I'm horrible with Mathematica :p
 
  • #47
TSny said:
Here's a video of the motion:

[I will delete this post if animations are not allowed to be uploaded or if it doesn't work for some reason. File size is 191.3 KB]

My thanks also!
 
  • #48
Great animation! One understands the problem at once when looking at it. You are a genius, TSny!

ehild
 
  • #49
TSny said:
Here's a video of the motion:

[I will delete this post if animations are not allowed to be uploaded or if it doesn't work for some reason. File size is 191.3 KB]

Great animation! I have one doubt regarding this, is it necessary that the time period of the revolutionary motion(the time taken to complete one revolution about the center) when viewed separately from the to and fro motion of the particle will be same as the time period of the to and fro motion?

In other words is it necessary that when the particle crosses say the x-axis it will always be at the same distance from the center? Or is that just a coincidence?
 
  • #50
consciousness said:
In other words is it necessary that when the particle crosses say the x-axis it will always be at the same distance from the center? Or is that just a coincidence?

Since the net force on an orbiting particle is an attractive inverse-square force, the motion of the particle will be an ellipse that does not precess. So, it will cross the x and y-axis at the same points each revolution.
 
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  • #51
TSny said:
Since the net force on an orbiting particle is an attractive inverse-square force, the motion of the particle will be an ellipse that does not precess. So, it will cross the x and y-axis at the same points each revolution.

Thanks!. This fact prompts me to search for an alternate solution to this problem.

If the four charges were revolving in a circular orbit initially and an impulse towards the central charge is provided to each simultaneously, would it be possible to get this exact situation?

If so would the time period of the motion change?(I tried to solve this problem by assuming that the time period doesn't change but got a wrong answer for my efforts)
 
  • #52
Thank you everyone for the help! :smile:

And nice animation TSny! :)
 
  • #53
consciousness said:
If the four charges were revolving in a circular orbit initially and an impulse towards the central charge is provided to each simultaneously, would it be possible to get this exact situation?

Yes. Since radial impulses will not change the angular momentum of the system, you would need to start in a circular orbit with the same angular momentum as for the final elliptical orbits.

If so would the time period of the motion change?(I tried to solve this problem by assuming that the time period doesn't change but got a wrong answer for my efforts)

Yes, the period will change. The radial impulses will increase the energy of the particles which will increase the period.
 
  • #54
I should have asked this earlier. Why a and b are the arithmetic and geometric means of the initial and final radii respectively?
 
  • #55
TSny said:
Yes, the period will change. The radial impulses will increase the energy of the particles which will increase the period.

I can confirm that. The time period for the initial circular orbit comes out be 0.0129 seconds, much less than that for the elliptical orbit. Why does increasing energy increase the time period?
 
  • #57
TSny said:
The radial impulses will increase the energy of the particles which will increase the period.
In what sense is the phrase energy being used here? Doesn't an elliptical orbit have less total energy than a circular orbit (zero for circular and negative for elliptical)?
 
  • #58
WannabeNewton said:
In what sense is the phrase energy being used here? Doesn't an elliptical orbit have less total energy than a circular orbit (zero for circular and negative for elliptical)?

Zero energy is in a parabolic orbit. For a circular orbit, zero pertains to eccentricity, not to energy. For any given angular momentum, energy is minimal for a circular orbit, which is easily seen from the equation relating eccentricity, energy, and angular momentum.
 
  • #59
voko said:
Zero energy is in a parabolic orbit. For a circular orbit, zero pertains to eccentricity, not to energy. For any given angular momentum, energy is minimal for a circular orbit, which is easily seen from the equation relating eccentricity, energy, and angular momentum.
Oops yeah I was mixing up eccentricity and energy. Cheers.
 
  • #60
consciousness said:
I can confirm that. The time period for the initial circular orbit comes out be 0.0129 seconds, much less than that for the elliptical orbit. Why does increasing energy increase the time period?

Total energy is directly related to the semi-major axis. This follows from considering conservation of energy and angular momentum at apoapsis and periapsis, try figuring that out.

The semi-major axis and period are related via Kepler's third law.
 
  • #61
consciousness said:
The time period for the initial circular orbit comes out be 0.0129 seconds, much less than that for the elliptical orbit.

I'm getting a period of .0456 s for the initial circular orbit. But I could have made a mistake.
 
  • #62
TSny said:
Here's a video of the motion:

[I will delete this post if animations are not allowed to be uploaded or if it doesn't work for some reason. File size is 191.3 KB]

A pretty picture, to be sure, but there is a lot of physics going on here:

a) Each mass is attracted by the other three gravitationally;
b) each mass is repelled by the other three electrostatically; and
c) each mass is attracted to the center charge electrostatically.
d) Then, an orbit of any kind requires a specific initial tangential velocity at a specific distance to determine that orbit.

Has your simulation provided for all these forces and initial velocities?

I note that if Gm2 = kq2, each of the four masses always has zero force on it due to the other three. Then each mass has an inverse-square force law as provided by its own charge q and that of the center charge -q. Unfortunately, I don't see Gm2 = kq2 as given.

So, again, have you accounted for all the forces and initial velocities?
 
  • #63
Gravitational force is completely negligible. If you care about the 5th decimal place, (EM) radiative effects would be way more important for any reasonable setup.

b) each mass is repelled by the other three electrostatically; and
c) each mass is attracted to the center charge electrostatically.
That gives the radial force.
d) Then, an orbit of any kind requires a specific initial tangential velocity at a specific distance to determine that orbit.
As you can see from the result, he took the right velocity to get the 4:1 distance variation.

I note that if Gm2 = kq2, each of the four masses always has zero force on it due to the other three.
That is wrong, both electrostatic and gravitational forces point inwards, they cannot add to zero. Anyway, gravity does not matter here.
 
  • #64
As mfb points out, the gravitational force is assumed to be neglected. Otherwise, you could not get a numerical answer based on the information given. [You could imagine an idealized system where the gravity and electrical forces are similar. For example, bowling balls with charges on the order of a nC. :smile:]

The important thing is that when you add up all of the electric forces on one of the moving particles, the net electric force is toward the central charge and varies as the inverse square of the distance r from the central charge: F = λ/r2. See post #1 where Pranav gives the explicit expression for λ.
 
  • #65
=Pranav-Arora;4446563]I should have asked this earlier. Why a and b are the arithmetic and geometric means of the initial and final radii respectively?[/QUOTE ]

Hi Pranav, see picture. The semi-major axis is 2a. 2a =r1+r2. For all points of the ellipse, the sum of distances from the foci has to be the same. The closest point to the left focus is A, at distance r1. The farthest point is at distance r2. A is at distance r1 from the left focus and at distance r2 from the right one. The sum of distances from the foci is r1+r2=2a. The sum of distances of point C from both foci is 2c=2a. So c=a. Form the yellow right triangle, b2=c2-(a-r1)2=a2-(a-r1)2=r1(2a-r1)=r1r2.

ehild
 

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  • #66
mfb said:
Gravitational force is completely negligible. If you care about the 5th decimal place, (EM) radiative effects would be way more important for any reasonable setup.
How do you know? m could be huge ... and the given constraint does not preclude a large m. Just make L0 small ...
That is wrong, both electrostatic and gravitational forces point inwards, they cannot add to zero. Anyway, gravity does not matter here.

The gravitational force between any two masses = Gm2/r2. This is an attractive force. The electrostatic force between the same two masses = kq2/r2. This is a repellent force. They cancel each other if Gm2 = kq2.
 
  • #67
rude man said:
How do you know? m could be huge ... and the given constraint does not preclude a large m. Just make L0 small ...
I know because it is a homework question, the central mass is not given and gravity is not mentioned.

The gravitational force between any two masses = Gm2/r2. This is an attractive force. The electrostatic force between the same two masses = kq2/r2. This is a repellent force. They cancel each other if Gm2 = kq2.
The central charge is negative, the outer charges are positive. If you add the forces, you get an attractive force. Please read the problem statement, it is explained there.
 
  • #68
mfb said:
I know because it is a homework question, the central mass is not given and gravity is not mentioned.
Unlike you, I and everyone else were not privy to that bit of information. I assumed the central mass = 0 but not the other four. I see no justification for that assumption. Once you mention "mass", gravity is kind of implied, is it not?

The central charge is negative, the outer charges are positive. If you add the forces, you get an attractive force. Please read the problem statement, it is explained there.

I acknowledge that if gravitational attraction is ignored then the remaining (electrostatic) forces are central. But I don't see ignoring gravity 'explained there'. :confused:

EDIT: in fact, I acknowledge that the forces are central even with the inclusion of gravity. But T cannot be determined without assuming zero gravitational attraction among the masses.
 
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  • #69
rude man said:
Unlike you, I and everyone else were not privy to that bit of information.
Actually, everyone else understood that gravity is supposed to be neglected.

I assumed the central mass = 0 but not the other four. I see no justification for that assumption.
Me neither.
Once you mention "mass", gravity is kind of implied, is it not?
No.

But T cannot be determined without assuming zero gravitational attraction among the masses.
Assuming zero, or neglecting it, right. Note that the problem statement said "particles". If those are elementary particles, gravity is weaker by ~40 orders of magnitude.
 
  • #70
kq2/mLo=104 was given. That means that gravitational force between two neighbouring particles is Fg=54q^2/Lo^6 and the electric force is 9˙109 q^2/Lo^2. The ratio Fg/Fe=6˙10-9 q^2/Lo^4 . Fg and Fe are comparable if q/Lo^2 is of the order 104, that is, the electric field of a particle at the position of its neighbour is about 1014 N/C.


ehild
 

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