How can the rotation of galaxies be explained?

In summary, the principle of spin conservation states that the total angular momentum of a system cannot be zero. This is why galaxies have a residual angular momentum even though the total angular momentum of the universe is not zero.
  • #1
Raimund Kempe
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How can galaxies rotate coming from a singularity?

Raimund
 
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  • #2
Raimund Kempe said:
How did you find PF?: Google search

How can galaxies rotate coming from a singularity?

Raimund
You apparently have a misconception of what "singualrity" means and you think it means a point in space where things came from. Even in pop-science it is not stated that galaxies came from a singularity but it is stated (incorrectly) that the universe exploded from a singularity.

Singularity just means "the place where our math model breaks down and we know know WHAT is/was going on".
 
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  • #3
Thanks for your response and the rectification, but the real question remains unanswered: How can galaxies' rotation be explained?

Raimund
 
  • #4
Raimund Kempe said:
How can galaxies' rotation be explained?
It is explained by Conservation of Angular Momentum.

  1. Take a volume of matter with random movement.
  2. Gravity draws the matter into clumps.
  3. The clumps retain the angular momentum of the original dust cloud, leaving a non-zero residual motion.
  4. Paths that do not intersect survive longer than paths that collide, leading to the gas cloud planing out and rotating in a common direction.
 
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  • #5
Thanks for bringing in this important principle of spin conservation.
Yet we have two questions:
What does this principle mean for the whole universe with its billions of rotating galaxies?
And what does it mean for the state at the very beginning?

Raimund
 
  • #6
Raimund Kempe said:
What does this principle mean for the whole universe with its billions of rotating galaxies?
nothing - the universe is not rotating - you seem to have reverted back to thinking that the universe "exploded" from a point in space.
And what does it mean for the state at the very beginning?
nothing - there was no rotation at the beginning - you seem to have reverted back to thinking that the universe "exploded" from a point in space and was somehow rotating then.

EDIT: think of a table on which there are a large number of spinning tops, some spinning one way, some the other way. Do you think that means that the table will rotate?
 
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  • #7
Your answers are not compatible to the principle of spin conservation.
The vector-sum of all galactic spins defines what could be called 'rotation'.
This vector-sum is not zero.

Raimund
 
  • #8
Perhaps it was a bad analogy. Do you think the entire universe is spinning? Do you realize that that would imply an axis that it is spinning about, which would imply a preferred frame of reference, thus negating the Cosmological Principle (the basis of modern cosmology)?
 
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  • #9
Raimund Kempe said:
Your answers are not compatible to the principle of spin conservation.
There is no such principle. There is conservation of angular momentum, but angular momentum includes more than just spin around centers of mass.
However, if we try to define the conserved angular momentum of the entire universe we run into the same sorts of problems that we encounter if we try to apply conservation of energy to the entire universe: the local differential formulation works just fine but the global integral formulation does not. The total angular momentum of the universe at a point in time is ambiguous for pretty much the same reasons that the total energy of the universe at a point in time is ambiguous.
 
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  • #10
Raimund Kempe said:
the real question remains unanswered: How can galaxies' rotation be explained?
I think you are confusing the angular momentum of an individual galaxy and the total angular momentum of the Universe. As far as I know, there is no evidence of any net angular momentum and no evidence of a 'preferred' axis but if you start with a sample of primordial gases (the future galaxy) then that sample would be expected to have a non zero angular momentum and some preferred axis. The rest follows.
 

1. What causes galaxies to rotate?

The rotation of galaxies is primarily caused by the gravitational pull of the massive amounts of dark matter and visible matter within the galaxy. As these objects move, they create a rotational force that causes the galaxy to spin.

2. How is the rotation of galaxies measured?

The rotation of galaxies can be measured using a variety of techniques, such as observing the Doppler shift of light from stars and gas within the galaxy, or analyzing the distribution of mass and velocity of objects within the galaxy.

3. Why do some galaxies rotate faster than others?

The rotation speed of a galaxy is dependent on its mass and distribution of mass. Galaxies with more mass and a more concentrated distribution of mass will rotate faster due to the stronger gravitational forces at play.

4. Can the rotation of galaxies be explained by the laws of physics?

Yes, the rotation of galaxies can be explained by the laws of physics, specifically the laws of gravity and motion. These laws govern the behavior of objects in the universe, including galaxies, and can accurately predict their rotational patterns.

5. Is the rotation of galaxies constant?

No, the rotation of galaxies is not constant. It can vary based on the distribution of mass within the galaxy, interactions with other galaxies, and the effects of dark matter. However, on a larger scale, the rotation of galaxies tends to follow predictable patterns and can be used to understand the structure and evolution of the universe.

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