Homework
Models of the Atom & Radioactivity
- Act 15A, p.173-176 Models of the Atom and Radioactivity
- Ex 5A, p. 151-155 Models of the Atom
- Ex 5B, p.160-171 Radioactivity
Nuclaer Reactions
- Act 16A, p. 181, Nuclear Reactions
- Ex 5C, p.175-182 Nuclear Reactions
Nuclear Reactions:
- Conservation of Atomic Number
- Conservation of Nucleon Number
- Conservation of Mass-Energy E = Δmc2
E = Δmc2
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
Element formation in Stars Nuclear Fusion
Binding Energy Per Nucleon
Mass Per Nucleon
A 'cheatsheet' on Binding Energy in nuclear physics
Binding Energy - A-level Physics
Nuclear Reactions
Fission Fusion and Radioactive Decay
Fission & Fusion
Natural Nuclear Fission Reactor
