Are supermassive black holes just big stars?

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Discussion Overview

The discussion revolves around the nature of supermassive black holes (SMBHs) and their potential relationship to massive stars. Participants explore whether SMBHs could originate from stars that grow large enough to prevent light from escaping due to their gravitational fields, and the implications of stellar mass and lifespan on black hole formation.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that a star could grow by consuming other stars until its gravitational field becomes so strong that light cannot escape, potentially leading to a state where it appears dark despite being hot and bright.
  • Others argue that as long as a star is shining, its volume would be too large to collapse into a black hole, suggesting that a star must exhaust its fuel before it can become a black hole.
  • There is a suggestion that if a sufficient mass is concentrated in a small volume, it could lead to black hole formation, but some participants question whether a black hole must already exist to prevent photons from escaping.
  • One participant notes that all wavelengths of light travel at the same speed, implying that if gravity can stop one wavelength, it can stop all, challenging the idea of a star dimming before becoming a black hole.
  • Concerns are raised about the lifespan of massive stars, with a participant mentioning that stars over 100 solar masses do not live long enough to accumulate significant additional mass, complicating the scenario of forming SMBHs from such stars.
  • A participant introduces the idea of primordial massive stars potentially being the progenitors of SMBHs, questioning if evidence exists in distant galaxies and whether SMBHs merely grew by accumulating stellar material over time.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the formation of SMBHs and the role of massive stars, with no consensus reached on whether supermassive black holes can form directly from large stars or if they require different mechanisms.

Contextual Notes

Participants highlight limitations in observational data regarding stellar collisions and the mass limits for star formation, indicating that the understanding of these processes is still developing.

Singlecoil
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Simple enough question. I know there are two types of black holes; the type formed after a star collapses in a supernova and the supermassive variety like the one at the center of the milky way.
If a star continued to grow by swallowing up other stars and solar systems is it possible that at a certain point its gravitational field would become so strong that light and heat could no longer escape? It would be a tipping point. Prior to reaching that mass it would be a bright star, but as it continued to grow it would start to dim as some wavelengths of the electromagnetic spectrum could no longer escape the massive star's gravitational field. Eventually it would reach such a size that it would appear dark to an observer, but in reality it is a bright and hot star that can no longer be conventionally detected.
 
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(Not absolutely sure.) As long as the star is shining its volume would be too big to become a black hole. Once it runs out of fuel then things would happen.
 
Seems likely that if you have enough mass in a small volume to keep photons from escaping, you have enough mass in a small volume that it will collapse into a black hole.

Or it may be that a BH has to already BE there to keep photons from escaping.
 
phinds said:
Seems likely that if you have enough mass in a small volume to keep photons from escaping, you have enough mass in a small volume that it will collapse into a black hole.

Indeed, this is a tautology by definition :)
 
Singlecoil said:
Prior to reaching that mass it would be a bright star, but as it continued to grow it would start to dim as some wavelengths of the electromagnetic spectrum could no longer escape the massive star's gravitational field.
All wavelengths of light travel at the same speed, if the gravity is enough to stop one then it can stop all.
 
I don't believe this is possible. Wouldn't an existing star simply burn more fuel, resisting collapse?
 
Drakkith said:
I don't believe this is possible. Wouldn't an existing star simply burn more fuel, resisting collapse?

If that were true, how would ANY BH ever form? I think I must be missing something about what you are saying.
 
phinds said:
If that were true, how would ANY BH ever form? I think I must be missing something about what you are saying.

I'm not saying that it wouldn't EVER turn into a black hole, only that it wouldn't be a black hole until it runs out of fuel.
 
The Jeans mass limits the 'birth' mass of stars [which varies for Pop 1, II and III stars]. The mass limit for coalescence of stars is not well known. Stellar collisions are so extraordinarily rare in the univerve we have insufficient observational data to model the upper limit for these events. One thing, however, is well established, enormously massive stars simply do not live long enough to accrete a large amount of additional mass. Stars more than 100 solar masses only live for tens of millions of years, as compared to the sun, which has a life expectancy of around ten billion years.
 
  • #10
Drakkith said:
I'm not saying that it wouldn't EVER turn into a black hole, only that it wouldn't be a black hole until it runs out of fuel.

Ah, I KNEW there was something I wasn't connecting the dots with. Thanks.
 
  • #11
Hello all,

As many of you have seen a few of my posts you will know I am not overly speculative, so I am in no way promoting this as a theory just want to know if anything along these lines has been pursued before:

I have read somewhere that the early U may have had enormous stars, in orders of magnitude larger than current stars, would it be possible that the SMBH's at the center of each galaxy formed from these primordial massive stars? Or would we see evidence of this in the most distant galaxies? Are there any predictions for what massive objects formed the SMBH's or are they considered to merely have grown due to being "fed" stellar material for a few billion years?

Any information is appreciated.
 
  • #12
Cosmo Novice said:
Hello all,

As many of you have seen a few of my posts you will know I am not overly speculative, so I am in no way promoting this as a theory just want to know if anything along these lines has been pursued before:

I have read somewhere that the early U may have had enormous stars, in orders of magnitude larger than current stars, would it be possible that the SMBH's at the center of each galaxy formed from these primordial massive stars? Or would we see evidence of this in the most distant galaxies? Are there any predictions for what massive objects formed the SMBH's or are they considered to merely have grown due to being "fed" stellar material for a few billion years?

Any information is appreciated.
The early stars were (order of magnitude) around 100 solar masses.

Black holes at galactic centers are of the order of millions to billions of solar masses. It seems unlikely that they could form from early stars without accumulating a lot more material.
 

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