Mercury Precession and the Hypothetical Oblate Sun Model

In summary: I forget what you're trying to say.The mass distribution in gas as a whole can still be more in the equator.In summary, the student thinks he is smarter than me and thinks he can disprove my theory that the sun is not oblate shape wise. He was talking about how the mass is distributed on the inside of the sun and how the tidal gravitational influence of the planets is insignificant compared to the oblateness from rotation. However, he does not have any evidence to back up his claim and it is incorrect.
  • #1
universityteacher
5
0
I have a student who thinks he is smarter than me.
When we calculate the precession the classical way we also account for the supposed oblate sun. If we model sun's oblateness by splitting the mass of the Sun into 2 masses and separate them by distance s, then the acceleration we get on point mass particle on x-axis is: a = - M/2 / [ (r + s)^2 ] - M/2 / [ (r - s)^2 ] and the equation that describe the motion takes on this form:
image024.gif

the ellipse will precess by 2(pi)PQ radians per revolution.

Now when we are modelling oblate sun (shape wise) we are actually modelling oblate sun mass wise. And so hypothetically if the sun is oblate enough (mass wise), then could we explain Mercury without Relativity.
I was telling him yes he could make this ridiculous claim and commit this blasphemy but he wouldn't get hired anywhere with that kind of attitude.
I was thinking of ways to prove that density of sun is not oblate (mass wise) and that we can use the shell theorem at will. Is there a way to prove our density of sun model or is his claim purely hypothetical at best?
 
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  • #2
Because it is a gas (plasma), mass would be spherically distributed, except for the effect of rotation. I presume this is not enough to account for the Mercury problem.
 
  • #3
I forgot to mention (sorry) that he was talking about mass moved to the equator by the pull of the planets (not Sun by itself). The problem here is that it looks like we cannot say for sure how the mass is distributed in the Sun.
 
  • #5
universityteacher said:
I was thinking of ways to prove that density of sun is not oblate (mass wise)

How is this different from proving that it isn't oblate shape wise?
 
  • #6
universityteacher said:
I forgot to mention (sorry) that he was talking about mass moved to the equator by the pull of the planets (not Sun by itself). The problem here is that it looks like we cannot say for sure how the mass is distributed in the Sun.
The tidal gravitational influence of the planets on the sun is well-known, and completely negligible compared to the oblateness from rotation. The oblateness from rotation is also well-known, and its contribution to the perihelion shift is negligible (less than 0.1% of the contribution from GR). Sure, you can discuss a tiny correction to a tiny effect, but it is utterly negligible.
 
  • #7
Dale said:
This is known as the solar quadrupole moment. Here is a good reference

http://cds.cern.ch/record/516377/files/0109032.pdf

mathman said:
except for the effect of rotation.
Is this what you mean by "known as the solar quadrupole moment?" Isn't that simulation done on a model of the Sun? The problem is we cannot know if mass is distributed spherically or oblately in the Sun. We have built a model of the Sun and are just running simulations on it.
 
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  • #8
universityteacher said:
The problem is we cannot know if mass is spherical or oblate in the Sun.
We know the mass is oblate, we know pretty well just how oblate it is, and we know how much that affects the orbit of Mercury.
 
  • #9
PeterDonis said:
How is this different from proving that it isn't oblate shape wise?
We might claim if the shape is round the mass distribution must also be round, but we're talking about gas(plasma). The mass distribution in gas as a whole can still be more in the equator. The problem here is we cannot know how it is on the inside.
 
  • #10
mfb said:
The tidal gravitational influence of the planets on the sun is well-known, and completely negligible compared to the oblateness from rotation. The oblateness from rotation is also well-known, and its contribution to the perihelion shift is negligible (less than 0.1% of the contribution from GR). Sure, you can discuss a tiny correction to a tiny effect, but it is utterly negligible.
mfb said:
The tidal gravitational influence of the planets on the sun is well-known
What do you mean by that? There could still be more mass in the equator. There could be or absolutely not? If there is than we can explain Mercury without Relativity.
 
  • #11
universityteacher said:
What do you mean by that? There could still be more mass in the equator. There could be or absolutely not? If there is than we can explain Mercury without Relativity.
Please read the material provided. The sun is oblate. We have both theoretical values and measured values for its quadrupole moment. Neither the theoretical nor the measured oblateness is sufficient to explain the precession of Mercury's orbit without relativity.

Please stop posting incorrect claims that have already been addressed.
 
  • #12
universityteacher said:
We might claim if the shape is round the mass distribution must also be round, but we're talking about gas(plasma).

The mass distribution will be more like the shape for a gas or plasma than it will for a liquid or especially a solid. In a gas or plasma there is effectively no internal force that prevents the mass distribution from adjusting itself to the effects of gravity, which is what determines the shape.
 
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  • #13
universityteacher said:
We might claim if the shape is round the mass distribution must also be round, but we're talking about gas(plasma). The mass distribution in gas as a whole can still be more in the equator. The problem here is we cannot know how it is on the inside.
We can know it, and we do know it.
A plasma is in hydrostatic equilibrium to an extremely good approximation (and we can measure the deviations). We also have helioseismography to probe the interior structure and we can use the differential rotation of poles and equators as cross-check. Multiple independent measurements all lead to consistent, small values for the quadrupole moment.
universityteacher said:
There could still be more mass in the equator.
Only within the uncertainties. The oblateness might be 20% smaller or larger than the current best estimate. But it is not a factor 1000 larger.
 
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1. What is Mercury precession and why is it important?

Mercury precession refers to the gradual change in the orientation of Mercury's orbit around the Sun. It is important because it helps us understand the dynamics of our solar system and can provide clues about the underlying forces at work.

2. What is the Hypothetical Oblate Sun Model?

The Hypothetical Oblate Sun Model is a theoretical model that suggests the Sun is not a perfect sphere, but rather is slightly flattened at the poles. This model was proposed to help explain the observed precession of Mercury's orbit, which could not be fully explained by Newtonian mechanics.

3. How does the Hypothetical Oblate Sun Model explain Mercury's precession?

The model proposes that the Sun's flattened shape causes it to have a non-uniform gravitational field, which in turn affects the orbit of Mercury. The varying gravitational pull from different parts of the Sun causes a torque on Mercury's orbit, leading to its observed precession.

4. Is the Hypothetical Oblate Sun Model widely accepted?

No, the Hypothetical Oblate Sun Model is still a controversial topic among scientists. While it has been able to partially explain Mercury's precession, it has not been able to fully account for all the observed data and there are alternative explanations that are still being explored.

5. Are there any other planets with observed precession similar to Mercury's?

Yes, Venus also has a slight precession in its orbit, but it is much smaller and can be fully explained by Newtonian mechanics. The precession of Uranus, however, has not been fully explained and is still a subject of study and debate in the scientific community.

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