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 of 4He?
Number of protons in 56 Fe = 26
Number of neutron in 56 Fe = 30
Energy of protons = 26 x mass of protons x 931.5 MeV ( since 1 amu = 931.5 MeV) = 26 x 1.007825 x 931.5 = 24408.5 MeV
Energy of neutrons= 30 x mass of neutrons x 931.5 MeV ( since 1 amu = 931.5 MeV) = 30 x 1.008665 x 931.5 = 28187.1 MeV
Energy of 56 Fe = 55.934937 x 931.5 MeV ( since 1 amu = 931.5 MeV) = 52103.4 MeV
Therefore Binding Energy = 28187.1 + 24408.5 - 52103.4 MeV = 492.2 MeV
Therefore Binding Energy per nucleon = 492.2 MeV / 56 = 8.789 MeV
Total energy released by one mole of 56 Fe = 6.023 x 1023 x 56 x 8.789 MeV = 2.964 x 1026 MeV
Binding energy of He can be calculated in a similar fashion and comes out to be 28.3 MeV
% of energy coming from the fusion of H to He = 28.3 x 100/ 492.2 = 5.75 %
Stellar nuclear fusion begins with 1H and ends with 56Fe. Younger stars fuse hydrogen to form...
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