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Are supermassive black holes just big stars? |
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| Dec15-11, 09:55 AM | #1 |
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Are supermassive black holes just big stars?
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. |
| Dec15-11, 03:11 PM | #2 |
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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.
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| Dec15-11, 03:15 PM | #3 |
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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. |
| Dec15-11, 04:01 PM | #4 |
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Are supermassive black holes just big stars? |
| Dec15-11, 04:18 PM | #5 |
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| Dec15-11, 07:48 PM | #6 |
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I don't believe this is possible. Wouldn't an existing star simply burn more fuel, resisting collapse?
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| Dec15-11, 07:59 PM | #7 |
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| Dec15-11, 08:29 PM | #8 |
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| Dec15-11, 09:23 PM | #9 |
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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.
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| Dec15-11, 10:18 PM | #10 |
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| Dec16-11, 06:11 AM | #11 |
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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. |
| Dec16-11, 03:32 PM | #12 |
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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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