One of the fusion reactions that goes on in massive stars is silicon burning, 28Si + 28Si→56Ni + γ. This reaction is how fusion reactions eventually reach the most stable iron/nickel region. It is also a precursor to the end of a star’s life and may lead to a supernova, if the star’s mass is suffi cient. (a) Calculate the ignition temperature required for this reaction. (b) How much energy is expended in this reaction?

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One of the fusion reactions that goes on in massive stars is silicon burning, 28Si + 28Si→56Ni + γ. This reaction is how fusion reactions eventually reach the most stable iron/nickel region. It is also a precursor to the end of a star’s life and may lead to a supernova, if the star’s mass is suffi cient.

(a) Calculate the ignition temperature required for this reaction.

(b) How much energy is expended in this reaction?

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