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IP Physics Notes (Upper Secondary, Year 3-4): 17) Radioactivity

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Trace nuclear structure, alpha/beta/gamma emissions, half-life maths, and safety protocols for IP nuclear physics.

Last updated 30 Nov 2025

Chee Wei Jie
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Chee Wei Jie·Academic Advisor (Physics)

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  1. Start Here
  2. Rutherford Scattering Recap
  3. Nuclear Notation & Isotopes
  4. Types of Radioactive Emission
Q: What does IP Physics Notes (Upper Secondary, Year 3-4): 17) Radioactivity cover?
A: Trace nuclear structure, alpha/beta/gamma emissions, half-life maths, and safety protocols for IP nuclear physics.
Quick recap -- Unstable nuclei shed energy by emitting alpha, beta, or gamma radiation. Identify the emission, update the nuclide notation, and use half-life reasoning to track activity changes.

Start Here

Read timeWhat to take away
1 secondRadioactivity is unstable nuclei changing by emitting radiation.
10 secondsAlpha changes mass and proton number, beta changes proton number, gamma changes energy only, and half-life halves activity after each equal time interval.
100 secondsUse the decay equations, half-life example, and safety notes to practise balancing nuclear notation, reading activity changes, and choosing shielding or handling methods.

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These notes align with SEAB GCE O-Level Physics (6091) content used in IP programmes (exams from 2026).

Status: SEAB O-Level Physics 6091 syllabus (exams from 2026) checked 2025-11-30 - scope unchanged; remains the reference for these notes.

Rutherford Scattering Recap

  • Most alpha particles passed straight through gold foil -> atoms mostly empty space.
  • Some deflected at large angles -> positive charge concentrated in tiny nucleus.
  • A few rebounded -> nucleus is dense and carries most mass.
  • Led to nuclear model: central nucleus (protons + neutrons) with orbiting electrons.