Once carbon is formed in massive star cores, the majority of nuclei formed form then on will belong to even numbered elements, due to addition to more helium nuclei as alpha particles.
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Q1: Because they all involve formation of iron
Q6: Iron nuclei are the most tightly bound
Q6: It takes less and less time to
Q7: A recurring nova could eventually explode as
Q10: Stellar nucleosynthesis is responsible for the existence
Q12: Iron is the most stably bonded atomic
Q15: Unlike supernovae, novae can explode more than
Q16: Type II supernovae have little hydrogen in
Q18: Newly formed neutron stars have weak magnetic
Q31: The element with the most stable nucleus
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