← Workshop GCSE Atomic Structure & Radioactivity

Atomic Structure & Radioactivity ☢️

From the nucleus to nuclear equations — interactive, animated, and with just enough humour to keep you from decaying.

AQA / Edexcel · GCSE Physics · Exam ready

⚛️ Inside the Atom

Protons, neutrons, and electrons — the original squad. Very small. Very important.

💬 "The atom is 99.9999% empty space. You are mostly nothing. Philosophical? Yes. Useful for exams? Also yes."
Element
Carbon
C
Mass Number A
12
Z + N
Charge
0
neutral atom
Colour key:
Protons positive charge +1 each
Neutrons no charge
Electrons negative charge −1 each
Where are they?
Protons + neutrons → nucleus (tiny, central, dense)
Electrons → shells/orbits around nucleus
Most of the atom: empty space

🔬 Isotopes & Ions

Same element, different story. Isotopes change the neutrons. Ions change the electrons.

Nuclear notation: ZX — where A = mass number (top), Z = proton number (bottom), X = element symbol.
Example: ¹²6C = Carbon-12 has 6 protons and 6 neutrons. ¹⁴6C = Carbon-14 has 6 protons but 8 neutrons.

🔴 Alpha Radiation (α)

A helium nucleus that decided to leave. Fast, heavy, easily stopped.

💬 "Alpha radiation is basically a helium nucleus that got angry and left. Stopped by a sheet of paper. Dangerous if inhaled — NOT from outside. Exam favourite."
Properties:
Composition: 2 protons + 2 neutrons (helium-4 nucleus)
Charge: +2
Mass: 4 u (heaviest radiation)
Ionising power: HIGH
Penetration: LOW — stopped by paper or skin
Nuclear equation rule:
A decreases by 4 (loses 2p + 2n)
Z decreases by 2 (loses 2 protons)

²³⁸92U → ²³⁴90Th + ⁴2He
Uranium-238 decays to Thorium-234
Deflection in fields: Alpha (+2 charge) deflects toward the negative plate in an electric field, and curves in a magnetic field according to the left-hand rule. Deflects more than beta (heavier).

🟠 Beta Radiation (β)

A neutron splitting into a proton, an electron, and an antineutrino. Messy but important.

Properties:
Composition: fast-moving electron (from nucleus)
Charge: −1
Mass: very small (~1/1840 of proton)
Ionising power: MEDIUM
Penetration: MEDIUM — stopped by ~5mm aluminium
Nuclear equation rule:
A stays the same (no change in mass number)
Z increases by 1 (neutron → proton)

¹⁴6C → ¹⁴7N + ⁰-1e
Carbon-14 decays to Nitrogen-14
Origin: A neutron in the nucleus transforms: n → p + e⁻ + antineutrino. The electron (beta particle) shoots out at high speed. Deflects opposite direction to alpha in electric fields (negative charge).

💜 Gamma Radiation (γ)

Pure electromagnetic energy. No mass, no charge, and it will go through most things like they aren't there.

Properties:
Composition: electromagnetic wave (photon)
Charge: 0 (not deflected by fields)
Mass: 0
Ionising power: LOW
Penetration: HIGH — needs thick lead or concrete
When does it happen?
Gamma is released AFTER alpha or beta decay. The daughter nucleus is in an excited state — it releases the excess energy as a gamma ray photon.

No change in Z or A — it's just energy loss.

Summary Comparison Table

Property Alpha α Beta β Gamma γ
Composition2p + 2n (He-4)Electron (e⁻)EM wave
Charge+2−10
IonisingHighMediumLow
PenetrationPaper / skin~5mm AlThick Pb/concrete
Deflected?Yes (+)Yes (−)No
Speed~5% cup to 90% cc (speed of light)

🛡️ Penetrating Power — Visual Comparison

The most common exam topic in this whole unit. Know it cold.

Exam tip: Barriers in order — paper, then aluminium (few mm), then thick lead (several cm), then thick concrete. Alpha stops at paper. Beta stops at aluminium. Gamma is only reduced (never truly zero) by thick lead/concrete.

⏱️ Half-Life

The time it takes for half the unstable nuclei in a sample to decay. Not all of them. Half. This distinction costs marks.

💬 "Half-life: the time for half the atoms to decay. NOT the time for ALL of them to be gone. Common exam mistake. Don't make it."
How to calculate half-life problems:
1. Find number of half-lives = total time ÷ half-life
2. Halve the starting amount that many times
Example: 800g, half-life = 10 years. After 30 years: 3 half-lives → 800 → 400 → 200 → 100g

Try a calculation

🔢 Nuclear Equations Builder

Both top numbers must balance. Both bottom numbers must balance. Every time.

Balancing rule: Mass numbers (top) on left = sum of mass numbers on right. Proton numbers (bottom) on left = sum of proton numbers on right. Check BOTH rows.

🌍 Background Radiation & Uses

Radiation is everywhere, all the time. Most of it is completely natural. Your granite worktop is mildly radioactive. This is fine.

Biggest source: Radon gas (from rocks and soil) accounts for ~50% of background radiation in the UK. It seeps into buildings from granite bedrock. Cornwall gets a lot of it.

Uses of Radioactivity

UseTypeWhy that type?
Medical tracers (PET scan)Gamma γPenetrates body, detected externally
Cancer radiotherapyGamma γKills cancer cells (targeted beam)
Sterilising medical equipmentGamma γKills bacteria without heat
Smoke detectorsAlpha αIonises air in chamber; smoke blocks it
Thickness gauging (paper mills)Beta βRight penetration for paper thickness
Carbon datingBeta βC-14 half-life ~5700 years

✅ Quiz — Test Yourself

5 questions. No pressure. Well. A little pressure. It's an exam topic.

1. Uranium-238 undergoes alpha decay. What are the mass number and proton number of the daughter nucleus?

2. A sample has an initial activity of 3200 Bq and a half-life of 8 years. What is the activity after 24 years?

3. Which type of radiation is stopped by a few millimetres of aluminium but passes through paper?

4. Two atoms are isotopes of each other. Which statement is correct?

5. What is the largest single source of background radiation in the UK?

☢️ Key Equations

A = Z + NMass number = protons + neutrons
N₀ → N₀/2 → N₀/4 → ...Activity halves every half-life
n = t / t½Number of half-lives = time ÷ half-life
α: A→A−4, Z→Z−2Alpha decay rule
β: A unchanged, Z→Z+1Beta decay rule
γ: no change to A or ZGamma = energy release only
²³⁸₉₂U → ²³⁴₉₀Th + ⁴₂HeAlpha decay example
¹⁴₆C → ¹⁴₇N + ⁰₋₁eBeta decay example
☢️ Radioactivity Tutor
Hi! I'm your GCSE radioactivity tutor. Ask me about nuclear equations, half-life calculations, penetration, isotopes — anything on this page. What do you want to tackle?