What determines the abundance of elements?

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SUMMARY

The abundance of elements in the universe is primarily determined by nuclear fusion processes occurring in aging stars and supernova explosions. While hydrogen and helium are abundantly produced during the Big Bang, heavier elements are synthesized through stellar fusion and dispersed during supernova events. The synthesis of elements like carbon occurs in the later stages of stellar evolution, while the rarity of elements such as boron and beryllium compared to cobalt can be attributed to their unique formation histories and the processes involved in stellar nucleosynthesis. Current models are improving but do not yet fully explain the complexities of elemental abundance.

PREREQUISITES
  • Understanding of stellar nucleosynthesis
  • Knowledge of supernova mechanisms
  • Familiarity with the periodic table and elemental properties
  • Basic concepts of astrophysics and cosmic evolution
NEXT STEPS
  • Research the process of stellar nucleosynthesis in detail
  • Study the mechanisms of supernova explosions and their role in element dispersal
  • Explore the formation and abundance of specific elements like boron and beryllium
  • Investigate current models of cosmic chemical evolution
USEFUL FOR

Astronomers, astrophysicists, students of cosmology, and anyone interested in the origins and distribution of elements in the universe.

martix
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I was just watching a very particular old documentary, when the question hit me.
I could probably manage an educated guess, but I don't really know what exactly determines how much of a certain element there is(except H and He, those are obvious).
 
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What is the source of other elements?
 
The source of all elements other than hydrogen, helium and some lithium is fusion in aging suns and supernovas. Fusion gets you to iron, but anything heavier is created during supernova explosions. We don't have a handle yet on the exact reactions involved or what controls the abundance, but models are getting better every year.
 
So... basically no answer to that question yet. :)
That's surprising.

I know that supposedly Carbon also gets produced at some point at the end phases of a stars life.

There's also the question why elements like boron or beryllium(4/5) are rarer than say cobalt(first element after iron, which is as far as I know that heaviest exothermally fusing element).
 
Actually the answer is here, you just have to think for a moment. My question was not a random one.

It is mainly a matter of the sample history. Metals (in astrophysics sense) are synthesized in stars, when (and if) the star explodes as supernova, they are scattered around, then they are included in the next generation stars, or separated due to the stratification in the gas clouds, and so on. Whatever you observe depends on what happened before.
 

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