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

Study guideUpdated 16 Jul 2026
Chee Wei Jie
Reviewed by
Chee Wei Jie·Academic Advisor (Physics)

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

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.

The core idea is simple: Radioactivity is unstable nuclei changing by emitting radiation.

Use it as a working check: Alpha changes mass and proton number, beta changes proton number, gamma changes energy only, and half-life halves activity after each equal time interval.

Then go one layer deeper: Use the decay equations, half-life example, and safety notes to practise balancing nuclear notation, reading activity changes, and choosing shielding or handling methods.

Keep your practice loop tight via our IP Physics tuition hub-it links each topic here to quizzes, diagnostics, and WA-style problem sets.

New to the Integrated Programme? Start with What is IP? | Browse all free IP notes.

For Integrated Programme students: Your current school materials, teacher instructions, and assessment scope take precedence because IP topic sequence and depth vary by school. This is an Eclat IP guide, not the O-Level / SEC G3 exam-track guide.

How this chapter applies

Sources

  1. National comparator - SEAB - 2027 SEC G3 Physics K323 syllabus
  2. MOE - Integrated Programme