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Which outcome limits iron-56 production inside aging massive stars?

A)Onset of reverse beta decay
B)Peak in nuclear binding energy
C)Neutron capture cross-section decline
D)Chandrasekhar mass limit exceeded

💡 Explanation

Thermonuclear fusion stops with iron-56 because adding nucleons requires energy rather than releasing it; this is because nuclear binding energy per nucleon peaks at iron-56. Therefore fusion cannot proceed past iron, rather than lighter elements, due to this energy requirement.

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