Thursday, 9 June 2016

Term 2 Week 6 2016

Homework,

  • Ex 5B Radioactive Decay and Half Life - This should be complete by now
  • Ex 5C Nuclear Reactions and Nuclear Energy Calculations - due next week
Nuclear Fusion in the Sun

Binding Energy comes from the change in mass from individual nucleons to being combined into a nucleus. This is energy lost by the nucleons joined together in a nucleus and must be returned in order to separate the nucleons
E = Δmc2

Mass Energy Equivalence

Nuclear Reactions

Fission Fusion and Radioactive Decay

Fission & Fusion


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