Stellar nuclear fusion begins with 1H and ends with
56Fe. Younger stars fuse hydrogen to form
4He, while older, more massive stars fuse Helium to form
heavier elements. Fusion beyond 56Fe is impossible
because iron-56 has the greatest binding energy per nucleon.
Calculate the binding energy per nucleon of 56Fe and use
it to calculate the maximum total energy per mole of
56Fe that could be released through nuclear fusion. What
percentage of the maximum total energy is released by the formation
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