Editing Talk:1123: The Universal Label
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[http://en.wikipedia.org/wiki/P-process] | [http://en.wikipedia.org/wiki/P-process] | ||
:The fusion of heavier elements is still fusion, even if it takes a supernova to make it happen. Nothing in the cartoon suggests that only the fusion reactions found in stable stars apply, and even more complicated processes (fusion+fission, whatever) involves matter that ultimately has a hydrogen pedigree. (I am, however, intrigued by the comment about helium and lithium in the early universe. I have some of those around here somewhere.) [[Special:Contributions/208.54.40.210|208.54.40.210]] 21:02, 19 October 2012 (UTC) | :The fusion of heavier elements is still fusion, even if it takes a supernova to make it happen. Nothing in the cartoon suggests that only the fusion reactions found in stable stars apply, and even more complicated processes (fusion+fission, whatever) involves matter that ultimately has a hydrogen pedigree. (I am, however, intrigued by the comment about helium and lithium in the early universe. I have some of those around here somewhere.) [[Special:Contributions/208.54.40.210|208.54.40.210]] 21:02, 19 October 2012 (UTC) | ||
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