How did we get elements above lead?

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Elements heavier than iron are primarily created through supernova nucleosynthesis, where the energy from a supernova explosion allows for the fusion of iron into heavier elements. Prior to this, elements up to iron are formed through fusion in stars, with iron having the highest binding energy per nucleon, making its fusion into heavier elements energy-intensive. The universe initially consisted mainly of hydrogen and helium, with only trace amounts of lithium and beryllium produced during the Big Bang nucleosynthesis, as there wasn't sufficient time for more complex elements to form. Discussions among scientists suggest that higher elements were not produced during the Big Bang, as the conditions were not conducive for their formation. Overall, the creation of elements above iron is a result of stellar processes and supernova events.
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This is something which has been a question to me that I don't seem to have stumbled across anything about myself:

How and when did/do the elements above Iron get created?

I've come across mention about the elements up to iron being generated by the process of fusion in stars. I assume you need bigger stars to fuse elements higher than hydrogen. Is that correct?

Does anyone here have info on how the elements above iron came/come to be?
 
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You're correct: iron has the highest binding energy per nucleon, so it costs energy to fuse it into heavier elements, and the end of the line for a heavy star (light stars usually have contracted long before this point) is theorized to be silicon burning:
http://en.wikipedia.org/wiki/Silicon_burning_process

At this point, the star either collapses into a neutron star, or a black hold, becoming a supernova in the process. The energy released in the process of blowing off the outer layers of the star supplies the energy required to fuse iron into heavier elements via supernova nucleosynthesis:
http://en.wikipedia.org/wiki/Supernova_nucleosynthesis

And hence the expression that we're all made of star dust. IANAAP (I am not an astrophysicist) however.
 
Thanks MAT
Any ideas on the energy difference in the fusion process itself and the energy generated in the blowing off process?
 
Sorry MAT. Only just read the link you provided. Thx for that.
It talks about what I asked.

Just another related question.
Is there any deliberation among scientists of the possibility of some production of higher elements during the high energies present during the big beginning.
Or is it considered to only have been an orderly process towards the production of hydrogen alone?
Did our universe initially only contain hydrogen until stars began to form or would there already have been some higher elements already present?
 
gonegahgah said:
Sorry MAT. Only just read the link you provided. Thx for that.
It talks about what I asked.

Just another related question.
Is there any deliberation among scientists of the possibility of some production of higher elements during the high energies present during the big beginning.
Or is it considered to only have been an orderly process towards the production of hydrogen alone?
Did our universe initially only contain hydrogen until stars began to form or would there already have been some higher elements already present?

According to conventional big bang models, the production of elements during the nucleosynthesis era of the universe was as follows:
75% Hydrogen
~25% Helium 4
.01% Deuterium
Trace amounts of lithium and beryllium

There just wasn't enough time to fuse anything more complex than that.

There's a lot of evidence to support the fact that this is the approximate element ratio pre-stellar nucleosynthesis, so it's quite accepted among scientists.

Reference: http://en.wikipedia.org/wiki/Big_Bang_nucleosynthesis
 
Thanks Nabe
 
In a typical Type II supernova, the newly formed neutron core has an initial temperature of about 100 billion kelvin (100 GK); 6000 times the temperature of the sun's core.

Source: http://en.wikipedia.org/wiki/SuperNova
 

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