Black Hole Formation and Iron Distribution

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Discussion Overview

The discussion revolves around the formation of black holes and the distribution of iron in the universe, particularly focusing on the contributions of supernovae to the iron content. Participants explore the origins of iron and carbon, the processes involved in supernova explosions, and the fate of stellar material during these events.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant inquires about the percentage of the universe's iron produced by supernovae that formed black holes, suggesting a range of 5 to 50%.
  • Another participant expresses interest in the origins of iron, noting that massive stars typically lose their iron during core collapse into neutron stars or black holes.
  • A participant asserts that heavy elements in nebulae are formed in the outer layers of stars, which are expelled during supernova explosions, while the core collapses into a black hole or neutron star.
  • Another participant emphasizes the role of Type Ia supernovae, which do not form black holes or neutron stars and release their entire mass, including iron group elements, into space.
  • It is mentioned that during core collapse, iron is destroyed due to the extreme heat, and new elements are formed in the ejecta of supernovae.

Areas of Agreement / Disagreement

Participants express varying views on the contributions of different types of supernovae to the iron content in the universe, and there is no consensus on the specific percentages or processes involved.

Contextual Notes

There are unresolved questions regarding the exact contributions of supernovae to the iron content and the mechanisms by which iron is produced and distributed in the universe.

nehorlavazapal
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Hi,

does anyone know how much of the universes's iron or carbon has been made in supernovae that formed black holes? Is it 5, 10, 50 % of the iron currently pressent here?

And, if se, do we have any idea how much of the average stars content gets traped in the BH versus the mass of the iron that gets out?
 
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Interesting question. I'd also like to know where most of the iron in the universe comes from since the most massive stars that produce it inside their cores typically lose it all when the cores collapse into neutron stars or black holes.
 
I was under the impression that the heavy elements in nebulae are made in the middle to outer layers that are blown off in the Supernova explosions. The core can collapse into BH or neutron star, and the outer layers (yet to be blown off) are bombarded briefly by vast quantities protons creating all sorts heavier than iron elements as well as the carbon, oxygen ect ect.


Damo
 
Damo ET said:
I was under the impression that the heavy elements in nebulae are made in the middle to outer layers that are blown off in the Supernova explosions. The core can collapse into BH or neutron star, and the outer layers (yet to be blown off) are bombarded briefly by vast quantities protons creating all sorts heavier than iron elements as well as the carbon, oxygen ect ect.


Damo

Yes, that's pretty much correct.
 
Don't forget Type-1A supernovae. These do not form black holes or neutron stars, so the entire mass of the supernova is blasted out into space. They typically form on the order of a solar mass of iron group elements, and they are quite common.
 
Also bear in mind that it doesn't much matter that there is iron in the core, other than the important fact that iron can't fuse and release energy, because the core gets so hot as it collapses that the iron is completely destroyed. A core-collapse pretty much reverses all the fusion processes that made the iron in the first place, so the fusion energy that is released as starlight is just a kind of "debt" that is repaid by gravitational energy during the collapse. But as has been said, new elements are fused in the ejecta (whether core-collapse or type Ia), so that's where the iron comes from.
 

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