Does the Spin of a Supermassive Black Hole Influence Its Galaxy's Rotation?

In summary: That may be debatable, Dave. Supermassive black holes are generally thought to form via mergers, and there is no telling how that affects spin. In any case, I doubt black hole spin has much effect on galactic rotation. There may be local frame dragging effects, but, is probably not significant on galactic scales.
  • #1
TRB8985
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My question is this:

Does the direction of spin of a supermassive black hole exert an affect on the spin of its surrounding galaxy (given that the above described black hole is at the center of such a galaxy)? Is there a direct or correlative effect? If so, can an in-depth explanation be provided?

Example:
The supermassive black hole at the center of the Milky Way galaxy spins clockwise. Therefore, the Milky Way spins clockwise. Is this true/false, and why?
 
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  • #2
Well, it's not that a BH will exert a force on the galaxy, but they will both almost certainly rotate in the same direction since they both form from the same rotating mass.
 
  • #3
That may be debatable, Dave. Supermassive black holes are generally thought to form via mergers, and there is no telling how that affects spin. In any case, I doubt black hole spin has much effect on galactic rotation. There may be local frame dragging effects, but, is probably not significant on galactic scales.
 
  • #4
Chronos said:
That may be debatable, Dave. Supermassive black holes are generally thought to form via mergers, and there is no telling how that affects spin.
Perhaps, but a merger will certainly result in a spherical galaxy rather than a spiral, so its "spin" won't be a meaningful term - for a few jillion years at least.
 
  • #5
Chronos said:
That may be debatable, Dave. Supermassive black holes are generally thought to form via mergers, and there is no telling how that affects spin. In any case, I doubt black hole spin has much effect on galactic rotation. There may be local frame dragging effects, but, is probably not significant on galactic scales.

Is this an issue of whether the SMBH forms before the spiraling starts in what end up being a spiral galaxy or after? That is, it seems to me that if the SMBH form AFTER the galaxy is basically spinning [which I recognize at probably unlikely], it would almost have to develop the same spin, whereas if it formed from collisions in the still more amorphous galactic center, then the subsequent galactic formation might NOT be related to the spin of the SMBH. Does that make sense?

Thanks
 
  • #6
i am an amateur at this stuff but, i believe that for a SMBH to form a very large body of mass larger than our sun needs to collapse inward. (ex. brown dwarf star) <--i think. so the body would already be spinning, thus the SMBH would acquire the same rotation at which it collapsed. (the mass' spin)
 
  • #7
MrGodParticle said:
i am an amateur at this stuff but, i believe that for a SMBH to form a very large body of mass larger than our sun needs to collapse inward. (ex. brown dwarf star) <--i think. so the body would already be spinning, thus the SMBH would acquire the same rotation at which it collapsed. (the mass' spin)

Perhaps, but that does not address the OP's question.
 
  • #8
Chronos said:
In any case, I doubt black hole spin has much effect on galactic rotation. There may be local frame dragging effects, but, is probably not significant on galactic scales.

This seems to be the most likely scenario.

Correct me if I'm wrong but doesn't the primary theory for SMBH's involve one being at the center of all galaxies? That being said, it seems like they (SMBH's) would be the reason galaxies form where they do, not the other way around.

It just doesn't feel right that galaxies (as we see them today) come before the SMBH. If that were the case I see no reason for a SMBH to be at the center of all galaxies instead of randomly distributed throughout the galaxy.
 
  • #9
Irish, I feel your view would be like saying the Sun was required to form before the gas cloud that collapsed to form the solar system in order for the gas cloud to collapse in the first place. I believe the galaxy as a whole (or rather its progenitor matter) began to collapse first, and the center of this collapsing cloud eventually formed the supermassive black hole.
 
  • #10
Heh okay when you put it like that my statement seems rather silly. On that note do galaxies need a SMBH at the center?
 
  • #11
Irishwake said:
Heh okay when you put it like that my statement seems rather silly. On that note do galaxies need a SMBH at the center?

Ah, that's a good question. Probably a Nobel prize in there if you can find the answer.

They all SEEM to have them, but it's not proven that all do, nor is it understood why they should or what the formation processes are.
 
  • #12
MrGodParticle said:
i am an amateur at this stuff but, i believe that for a SMBH to form a very large body of mass larger than our sun needs to collapse inward. (ex. brown dwarf star) <--i think. so the body would already be spinning, thus the SMBH would acquire the same rotation at which it collapsed. (the mass' spin)

A brown dwarf is a "star" much smaller than our Sun which is not massive enough to fuse protons via the proton-proton chain, but massive enough to fuse deuterium. They are usually ~12 Jupiter masses to something like .35 solar masses if I remember correctly.

Because SMBH's are so much more massive than any star that we know of (some 10^8 or more solar masses), it doesn't seem plausible that such a massive "star" existed in the first place. SMBH's are almost certainly the result of many mergers of smaller black holes. How that can occur, given the dynamic time scales for galactic motion compared to the age of the universe, is not well understood. The universe doesn't seem to be old enough to have formed black holes of these sizes through "conventional" methods.
 
  • #13
While a common theory is that supermassive black holes formed by accretion of dust and then stars into an initial black hole, there is no reason this is necessary. The total density of a SMBH is not particularly large (a billion star SMBH has a density measured at horizon of 1% that of water). One could imagine a central mass of a billion stars, slowed by dust, slowly coalescing to this density.
 
  • #14
PAllen said:
One could imagine a central mass of a billion stars, slowed by dust, slowly coalescing to this density.

One can imagine, but I'm not sure this is physically realizable. What differentiates such a scenario from standard star formation (which obviously does not generate extraordinarily large black holes)?
 
  • #15
I see no obvious reason galactic spin need align with that of its central SMBH. Even assuming the SMBH forms first, how does that dictate the spin of a galaxy that eventually spans hundreds of thousands of light years? I think the dark matter halo makes more sense.
 
  • #16
Nabeshin said:
One can imagine, but I'm not sure this is physically realizable. What differentiates such a scenario from standard star formation (which obviously does not generate extraordinarily large black holes)?

It would have nothing to do with star formation. It would occur in well formed galaxies with large central star clusters. In fact, if a few stars happen to become black holes, I don't see how that changes the dynamics of the cluster. Once there is something (and it seems there must be) to allow sufficient exchange of angular momentum, it shouldn't matter whether you have stars or small black holes coalescing.

Anyway, this is just a speculation; but so are all accounts of SMBH formation that I've read.
 
  • #17
PAllen said:
It would have nothing to do with star formation. It would occur in well formed galaxies with large central star clusters. In fact, if a few stars happen to become black holes, I don't see how that changes the dynamics of the cluster. Once there is something (and it seems there must be) to allow sufficient exchange of angular momentum, it shouldn't matter whether you have stars or small black holes coalescing.

Anyway, this is just a speculation; but so are all accounts of SMBH formation that I've read.

I see, sorry, I thought for some reason by your post that you meant direct collapse of a million solar mass cloud of gas into a SMBH (which I think we'll agree is impossible).
 

FAQ: Does the Spin of a Supermassive Black Hole Influence Its Galaxy's Rotation?

What is the rotation of a black hole?

The rotation of a black hole refers to the spinning motion of a black hole. Just like planets and stars, black holes can also rotate due to their angular momentum. This rotation causes the black hole to have a slightly oblong shape.

How does the rotation of a black hole affect its gravitational pull?

The rotation of a black hole affects its gravitational pull by creating a phenomenon called frame-dragging. This means that the rotation of the black hole causes spacetime to twist around it, which affects the motion of objects and particles near the black hole.

Can a black hole rotate at any speed?

Yes, black holes can rotate at any speed, including near the speed of light. However, the maximum speed at which a black hole can rotate is determined by its mass and angular momentum.

What is the significance of the event horizon in the rotation of a black hole?

The event horizon is the boundary around a black hole from which nothing, not even light, can escape. The rotation of a black hole affects the shape and size of its event horizon, which can also affect the rotation of matter and energy that falls into the black hole.

How does the rotation of a black hole affect its lifespan?

The rotation of a black hole does not have a significant impact on its overall lifespan. However, a rotating black hole can emit energy through a process called the Penrose process, which can cause the black hole to lose its rotational energy and eventually stop rotating. This could, in turn, affect the black hole's lifespan.

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