How Are Elements Beyond Iron Created in Stars?

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The discussion centers on the creation of elements beyond iron in stars, highlighting that iron fusion marks the end of a massive star's life cycle. Stars can fail to reach the iron stage if they lack sufficient mass, and those that do will form iron cores within about a day before imploding due to gravity. This implosion leads to a supernova explosion, during which new elements are formed through a process known as the r-process, where iron nuclei are coated with neutrons. Some of these neutrons decay into protons, resulting in the creation of new elements. The conversation raises questions about the specifics of this "coating" and its implications for element formation.
solarblast
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A friend wrote this in an exchange we had about iron and its role in the process of fusion. I question the last sentence. Is it right, and what is the "coating"?

The creation of the element iron via fusion "is the final peal of a star's natural life" (if the star is massive enough to even get that far -- stars can peter out long before they reach the iron stage if the star is not massive enough to begin with) . After burning down through all the elements up to iron, these stars burn down to iron cores in about one Earth day. And then, suddenly lacking the energy to fuse to higher elements and to keep their full volume, they implode under immense gravity and then rebound by exploding outward into an immense supernova. It is in this process that the remaining elements are born by coating iron nuclei with neutrons, some of which decay back into protons thereby creating new elements.
 
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This is called the r-process. But, it's not just iron nuclei that get neutron enriched by this process.
 

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