Galaxy rotation and light bending

In summary: The observed galaxy rotation curves are a puzzle. I can't see how gravitational lensing can play a part in this - can you provide a model ? Maybe frame dragging also produces a doppler effect ?The literature is infested with articles claiming to have solved the rotation curve anomaly, but so far nothing really hits the spot.Your wiki reference says:Dark matter also correctly predicts the results of gravitational lensing observations.
  • #1
lalbatros
1,256
2
Hello,

Reading a news on Yahoo, I was asking myself a little question.

I assume there are today extensive data about galaxies rotation as well as light bending by the same galaxies.
The question is: how consistent are these data?
The rotation curve of a galaxy is known to be flatter than "expected"
300px-GalacticRotation2.svg.png

(http://en.wikipedia.org/wiki/Galaxy_rotation_problem).
Would that also imply something about the light bending from the same galaxy?
Would that imply a lower bending of light or a higher bending of light?
And what are the experimental data and correlations?
And are the experimental data consistent with the expectations?

Thanks
 
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  • #2
The observed galaxy rotation curves are a puzzle. I can't see how gravitational lensing can play a part in this - can you provide a model ? Maybe frame dragging also produces a doppler effect ?

The literature is infested with articles claiming to have solved the rotation curve anomally, but so far nothing really hits the spot.
 
  • #3
Your wiki reference says:
Dark matter also correctly predicts the results of gravitational lensing observations.

So are your questions related to how closely these lensing observations meet theoretical predictions?

As you likely know, galactic stars some distance from galactic centers do not appear to rotate at expected speeds based on visible matter...to explain the spiral galaxy rotational velocities additional dark matter (mass) is required in the outer portions of galaxies...more mass curves light more but how the closely observational data correlates to various dark mass distribution proposals I don't know. And it could vary for different galaxy types.

THE TROUBLE WITH PHYSICS, by Lee Smolin discusses discuss galactic velocity mass/velocity discrepancies beginning pg 210. He notes
In each galaxy where the problem is found it affects only stars moving outside a certain oribit...at a certain distance from the center? No...at a certain star density? no..As one moves further out from the center of a galaxy..there turns out to be a critical acceleration rate that marks the breakdown of Newton's law of gravity...its close to c^2/R, (R is the scale of the observable universe) the cosmological constant! (Discovered in the 1980's it's now called Milgrom's law...his theory: MOND in the Wikipedia article)...MOND does not work outside galaxies...does not make much sense to physicsts...works within about 80 of 100 galaxies studies..

Smolin footnote: More on MOND and supporting data: www.astro.umd.edu/~ssm/mond/.
 
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1. What causes galaxies to rotate?

Galaxies rotate due to the conservation of angular momentum. As a galaxy forms, the rotation of the cloud of gas and dust from which it is born is amplified and maintained as the galaxy grows. This rotation is also influenced by the gravitational pull of neighboring galaxies.

2. How does the rotation of a galaxy affect the light it emits?

The rotation of a galaxy can affect the light it emits in a few ways. Firstly, the rotation can cause the light to be redshifted or blueshifted, depending on the direction of rotation and the observer's perspective. Additionally, the rotation can cause the light to be distorted or bent as it travels through the galaxy's gravitational field.

3. Why do galaxies appear to bend light?

Galaxies bend light due to the effects of gravity. As light travels through the gravitational field of a galaxy, its path is altered, causing it to appear to bend. This phenomenon is known as gravitational lensing and is a result of Einstein's theory of general relativity.

4. How do scientists study galaxy rotation and light bending?

Scientists study galaxy rotation and light bending through various methods, such as observing the Doppler effect on emitted light, measuring the rotation curves of galaxies, and analyzing the distortion of light from distant objects due to gravitational lensing. These methods allow scientists to gather data and make predictions about the structure and behavior of galaxies.

5. What can the study of galaxy rotation and light bending tell us about the universe?

The study of galaxy rotation and light bending can provide valuable insights into the structure and evolution of the universe. By understanding how galaxies rotate and how their gravitational fields affect light, scientists can better understand the distribution of dark matter and the expansion of the universe. This research also helps us to better understand the laws of gravity and the fundamental principles that govern our universe.

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