This mini-lesson walks you through the whole of Eduqas Topic 9 — Atomic structure: the nuclear atom & isotopes, how the model developed, the absorption & emission of ionising radiations, hazards and uses of radioactivity, and nuclear fission & fusion.
Almost all of the atom is empty space; nearly all its mass sits in the tiny central nucleus.
Work through each screen, answer the questions as you go (some are wordy, some are calculations) and collect ⭐ stars. Purple HT tags mark Higher-tier-only content. Press Start when you're ready.
Nuclear atom and isotopes
Inside the atom
Atoms are about 1 × 10⁻¹⁰ m across, but the nucleus at the centre is around 10 000 times smaller (~1 × 10⁻¹⁴ m). The nucleus holds the protons and neutrons; the electrons occupy energy levels around it.
Protons and neutrons have almost all the mass; the electron's mass is negligible.
Watch out: an atom is neutral because the number of protons equals the number of electrons. Lose or gain electrons and it becomes a charged ion.
Nuclear atom and isotopes
Numbers, notation & isotopes
Atomic number (Z) = number of protons (it defines the element).
Mass number (A) = number of protons + neutrons.
Number of neutrons = A − Z.
Isotopes are atoms of the same element (same Z) with different numbers of neutrons (different A).
Nuclide notation: the top number is the mass number A, the bottom is the atomic number Z.
Common slip: isotopes do not differ in protons or electrons — only in neutrons. They behave the same chemically but can differ in nuclear stability.
Quick check
Counting the nucleus
?An atom is written as oxygen-17 with atomic number 8. How many neutrons does it contain?
Nuclear atom and isotopes
How the model developed
Our picture of the atom changed as new evidence arrived:
Plum pudding model — a ball of positive charge with electrons dotted through it (no nucleus).
Alpha-scattering experiment — alpha particles fired at thin gold foil. Most passed straight through, but a few were deflected and some bounced back.
Nuclear model — this proved the atom is mostly empty space with a tiny, dense, positively charged nucleus.
The few alpha particles that bounced back showed the positive charge and mass are concentrated in a tiny nucleus.Absorption & emission of ionising radiations
Electron energy levels
Electrons occupy fixed energy levels around the nucleus. They can move between levels by gaining or losing energy as electromagnetic radiation:
Absorption — an electron absorbs EM radiation and jumps up to a higher energy level.
Emission — an electron emits EM radiation and drops down to a lower energy level.
The same idea, taken further, becomes the Bohr model of fixed orbits (Higher tier).
HTThe refined Bohr model — electrons orbiting at set distances — is Higher-tier only.
Absorption & emission of ionising radiations
Three types of nuclear radiation
An unstable nucleus becomes more stable by emitting ionising radiation. There are three kinds:
Beta (β) — a fast electron emitted when a neutron turns into a proton. Charge −1.
Gamma (γ) — high-energy electromagnetic radiation from the nucleus. No mass, no charge.
Penetration: α stopped by paper · β stopped by a few mm of aluminium · γ only reduced by thick lead (or concrete).
Key misconception: alpha is the most ionising but the least penetrating (it bumps into atoms easily). Gamma is the least ionising but the most penetrating. Ionising power and penetration run in opposite orders.
Sort it
Which radiation?
Tap the type of radiation that matches each clue.
Absorption & emission of nuclear particles
Nuclear decay equations
In any decay, the total mass number and the total charge (atomic number) are conserved — they must balance on both sides.
α decay: AX → A−4Y + 4Hemass number drops by 4, atomic number drops by 2 (an alpha particle leaves)
β decay: AX → AY + 0emass number unchanged, atomic number rises by 1 (a neutron → proton + electron)
Worked example — alpha decay of radium-226
²²⁶₈₈Ra → ²²²₈₆Rn + ⁴₂He
Mass: 222 + 4 = 226 ✓ Charge: 86 + 2 = 88 ✓
Remember: in beta decay the mass number stays the same (the electron has mass number 0), but the atomic number goes up by 1 because a neutron became a proton.
Balance it
Your turn — alpha decay
1Uranium-238 (atomic number 92) emits an alpha particle. What is the mass number of the new thorium nucleus that forms?
mass number
Hint: alpha decay lowers the mass number by 4 → 238 − 4.
Balance it
Your turn — beta decay
2Carbon-14 (atomic number 6) undergoes beta decay to form nitrogen. What is the atomic number of the nitrogen nucleus?
atomic number
Hint: beta decay raises the atomic number by 1 → 6 + 1.
Absorption & emission of ionising radiations
Activity & half-life
Radioactive decay is a random process — you cannot say which nucleus decays next. But for a large sample, the rate is predictable. The activity (measured in becquerels, Bq) is the number of decays per second.
The half-life is the time taken for the number of unstable nuclei (or the count-rate) to halve.
Each half-life the count-rate halves: 100 → 50 → 25 → 12.5. The curve never quite reaches zero.
HTMisconception: half-life is probabilistic, not a countdown for one atom. It does not mean the sample is gone after two half-lives — after 2 half-lives a quarter remains; after 3, an eighth.
Calculate
Your turn — half-life
3A source has a half-life of 6 hours. A sample starts at a count-rate of 800 counts/min. What is the count-rate after 18 hours?
4A radioactive sample falls to one quarter of its original count-rate in 40 minutes. What is its half-life, in minutes?
minutes
Hint: a quarter means 2 half-lives have passed. 40 ÷ 2 = ?
Hazards and uses · background radiation
Background radiation
We are exposed to low-level background radiation all the time. It comes from natural and man-made sources:
Most background radiation is natural — radon gas from rocks is the single biggest contributor in many areas.
When measuring a source's activity, you must subtract the background count first to get the true reading.
Hazards and uses of radioactive emissions
Hazards: irradiation vs contamination
Ionising radiation is dangerous because it can damage cells and DNA. There are two distinct hazards:
Irradiation — being exposed to radiation from an outside source. The object/person does not become radioactive, and it stops when the source is removed.
Contamination — radioactive atoms get onto or into an object. They keep decaying there, so the hazard continues.
Safety: keep your distance, limit time of exposure, and use shielding (lead, concrete) and protective clothing. Store sources in lead-lined boxes.
HTDon't mix them up: irradiation ≠ contamination. Inside the body, an alpha source is the most dangerous (highly ionising, all energy dumped locally). Outside the body, gamma/beta are more hazardous because alpha can't penetrate skin.
Hazards and uses of radioactive emissions
Uses of radioactivity
The properties of each radiation make it useful in different ways:
Medical tracers — a gamma source with a short half-life is swallowed/injected and tracked outside the body (e.g. PET scans).
Sterilisation — gamma kills microbes on medical equipment and food without heating them.
Treating cancer — targeted gamma "radiotherapy" destroys tumour cells.
Smoke detectors — an alpha source; smoke absorbs the alpha and trips the alarm.
Radioactive dating — carbon-14 dating of once-living material; uranium dating of rocks.
Thickness control — a beta source monitors the thickness of paper/foil in a factory.
Why those choices? The penetration of each type decides its job — gamma to pass out of the body, alpha (short range) for a smoke alarm, beta for thickness gauges (partly absorbed by the sheet).
Match up
Match the use to the radiation
Tap a use on the left, then its best-matched radiation on the right.
Nuclear fission and fusion
Nuclear fission
Nuclear fission is the splitting of a large, unstable nucleus (e.g. uranium-235) into two smaller nuclei, releasing 2 or 3 neutrons, gamma rays and a lot of energy.
Each fission releases neutrons that can trigger more fissions — a chain reaction.
HTIn a reactor a chain reaction must be controlled: control rods (e.g. boron) absorb spare neutrons to set the rate, and a moderator slows neutrons down so they are absorbed.
Nuclear fission and fusion
Nuclear fusion
Nuclear fusion is the joining of two small, light nuclei (e.g. hydrogen) to make one larger nucleus, releasing energy. This is the process that powers stars, including the Sun.
Fusion: small nuclei join to release energy — the opposite of fission.
HTFusion needs extremely high temperature and pressure so nuclei move fast enough to overcome the electrostatic repulsion between their positive charges — which is why it is so hard to do on Earth.