Retrieving "Stellar Nucleosynthesis Of Carbon" from the archives

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1. Neon 22

   Linked via "carbon burning stages"

   Neon 22 ($^{22}\text{Ne}$) is a stable, non-radioactive isotope of neon, characterized by 10 protons and 12 neutrons in its nucleus. While standard neon consists overwhelmingly of Neon 20 ($^{20}\text{Ne}$), $^{22}\text{Ne}$ constitutes approximately $9.24\%$ of naturally occurring neon in terrestrial atmospheres [1]. This isotopic abundance is significantly higher in certain stellar environments, particularly…