GCSE Physics

AQA GCSE · Physics 8463 · course summary

Physics 8463.

The separate science GCSE on one page: the two exam papers, then everything in the eight topics, with the equations and the ten required practicals.

An unofficial summary of the AQA GCSE Physics specification (8463, version 1.1), shortened and in my own words. It is not an AQA publication. For the exact wording, read the specification itself.

1 Exam format

Two written papers, both sat at the end of the course. Students sit both at the same tier, Foundation or Higher.

PaperTopicsTimeMarksWeight
Paper 11 Energy, 2 Electricity, 3 Particle model of matter, 4 Atomic structure1 h 45 min10050%
Paper 25 Forces, 6 Waves, 7 Magnetism and electromagnetism, 8 Space physics. May also draw on energy transfers and conservation from topics 1 and 2.1 h 45 min10050%
Total3 h 30 min200100%

Question types

Multiple choice, structured, closed short answer and open response. Extended answers may be prose, a long calculation, or both.

Tiers and grades

Grades 9 (best) to 1. Foundation tier gives grades 1 to 5; Higher tier gives 4 to 9, with an allowed grade 3 for a near miss. Below that is U.

Assessment objectives

  • AO1 knowledge and understanding · about 40%
  • AO2 applying it · about 40%
  • AO3 analysing, evaluating, improving methods · about 20%

Practical skills

At least 15% of the marks come from questions on the required practicals. There is no coursework.

Equations sheet

Every physics paper comes with the AQA Physics Equations Sheet, so the equations below need not be memorised; the one exception is \(R_{\mathrm{total}} = R_1 + R_2\). (AQA notice)

Linear

Both papers are sat in the same May/June series at the end of the course. Raw marks are added together and the grade is set on the total out of 200.

2 Subject content

Eight topics, in the specification’s order and numbering. Content marked Physics only is the extra for the separate science; dashed boxes are physics only in full.

4.1Energy

Paper 1

4.1.1Energy stores and systems

  • A system is an object or a group of objects; describe how the energy stored changes when a system changes (a ball thrown up, a car braking, a kettle boiling).
  • Calculate energy changes caused by heating, by forces doing work and by an electric current.
  • Kinetic, elastic potential and gravitational potential energy.
  • Specific heat capacity: the energy to raise 1 kg by 1 °C.
  • Power as the rate of transferring energy or doing work; 1 W is 1 J/s.
  • \(E_{\mathrm{k}} = \tfrac{1}{2}mv^2\)
  • \(E_{\mathrm{e}} = \tfrac{1}{2}ke^2\)
  • \(E_{\mathrm{p}} = mgh\)
  • \(\Delta E = mc\Delta\theta\)
  • \(P = \dfrac{E}{t}\)
  • \(P = \dfrac{W}{t}\)

Required practical 1 · specific heat capacity

4.1.2Conservation and dissipation

  • Energy is never created or destroyed; in a closed system the total stays the same.
  • Some energy is always dissipated into less useful stores (“wasted”); reduce it with lubrication and thermal insulation.
  • Higher thermal conductivity means faster conduction; how wall thickness and conductivity affect how fast a building cools.
  • Efficiency as a decimal or a percentage.
  • HT Ways to make an energy transfer more efficient.
  • \(\text{efficiency} = \dfrac{\text{useful output energy}}{\text{total input energy}}\)
  • \(\text{efficiency} = \dfrac{\text{useful power output}}{\text{total power input}}\)

Required practical 2 Physics only · thermal insulators

4.1.3National and global energy resources

  • Fossil fuels, nuclear fuel, bio-fuel, wind, hydroelectricity, geothermal, tides, the Sun and water waves.
  • Renewable against non-renewable; reliability; uses in transport, electricity generation and heating.
  • Environmental impact, and trends in how resources are used.
  • Science can identify the problems but political, social, ethical and economic factors limit what is done.
  • How each resource generates electricity is not needed.

4.2Electricity

Paper 1

4.2.1Current, potential difference and resistance

  • Draw and read circuit diagrams with standard symbols.
  • Current is the rate of flow of charge, and is the same all round a single loop.
  • Ohmic conductors at constant temperature; non-constant resistance of filament lamps, diodes, thermistors and LDRs, and their uses (thermostats, lights that switch on at dusk).
  • Measuring resistance with an ammeter and voltmeter; reading I–V graphs.
  • \(Q = It\)
  • \(V = IR\)

Required practicals 3 · resistance, and 4 · I–V characteristics

4.2.2Series and parallel circuits

  • Series: same current, p.d. shared, resistances add.
  • Parallel: same p.d., currents add, total resistance less than the smallest resistor.
  • Explain why adding resistors in series raises the total and in parallel lowers it.
  • Calculations in series circuits; the total of two resistors in parallel is not calculated.
  • \(R_{\mathrm{total}} = R_1 + R_2\) (not on the sheet)

4.2.3Domestic uses and safety

  • Direct and alternating p.d.; UK mains is ac at 50 Hz and about 230 V.
  • Three-core cable: live (brown), neutral (blue), earth (green and yellow).
  • Why a live wire is dangerous even with the switch open, and why any connection between live and earth is dangerous.

4.2.4Energy transfers

  • Power of a device from p.d. and current, or from current and resistance.
  • Energy transferred depends on power and time switched on; appliances transfer energy to motors and heaters.
  • The National Grid: step-up transformers for transmission, step-down for homes, and why this is efficient.
  • \(P = VI\)
  • \(P = I^2R\)
  • \(E = Pt\)
  • \(E = QV\)

4.2.5Static electricity Physics only

  • Rubbing insulators transfers electrons: the gainer turns negative, the loser equally positive.
  • Like charges repel, unlike attract, without contact; sparking.
  • Electric fields: strongest near the charge; the field of an isolated charged sphere; how fields explain the forces and sparks.

4.3Particle model of matter

Paper 1

4.3.1Changes of state and density

  • Particle diagrams of solids, liquids and gases, and how they explain differences in density.
  • Melting, freezing, boiling, evaporating, condensing and subliming conserve mass; they are physical changes, reversed to get the original material back.
  • \(\rho = \dfrac{m}{V}\)

Required practical 5 · density

4.3.2Internal energy and energy transfers

  • Internal energy is the total kinetic and potential energy of all the particles.
  • Heating raises the temperature or changes the state.
  • Specific latent heat of fusion and of vaporisation: energy for a change of state with no change in temperature.
  • Heating and cooling graphs; telling specific heat capacity and latent heat apart.
  • \(\Delta E = mc\Delta\theta\)
  • \(E = mL\)

4.3.3Particle model and pressure

  • Gas molecules move randomly; temperature relates to their average kinetic energy.
  • At constant volume, a hotter gas exerts a higher pressure.
  • Physics only Pressure gives a force at right angles to the walls; at constant temperature a larger volume means a lower pressure.
  • Physics only HT Doing work on a gas (a bicycle pump) raises its temperature.
  • \(pV = \text{constant}\) Physics only

4.4Atomic structure

Paper 1

4.4.1Atoms and isotopes

  • Atom radius about \(1 \times 10^{-10}\) m; nucleus under \(\dfrac{1}{10\,000}\) of that but holding almost all the mass.
  • Electrons in energy levels move up by absorbing and down by emitting electromagnetic radiation.
  • Atomic number, mass number, isotopes and positive ions.
  • How the model changed: solid spheres, plum pudding, the nuclear model from alpha scattering, Bohr’s orbits, protons, Chadwick’s neutron.

4.4.2Atoms and nuclear radiation

  • Unstable nuclei decay at random; activity in becquerels; count rate.
  • Alpha, beta, gamma and neutron emission; penetration, range in air and ionising power, and choosing a source for a job.
  • Balanced nuclear equations for single alpha and beta decays.
  • Half-life, found from data or a graph. HT The fraction left after a number of half-lives, as a ratio.
  • Contamination against irradiation; why studies of radiation effects are published for peer review.

4.4.3Hazards and uses of radiation Physics only

  • Background radiation from rocks and cosmic rays, and from weapons tests and nuclear accidents; dose depends on job and location.
  • Half-lives range widely, which changes the hazard.
  • Medical uses: exploring internal organs and destroying unwanted tissue; weighing perceived risk against data.

4.4.4Nuclear fission and fusion Physics only

  • Fission of uranium or plutonium, usually after absorbing a neutron: two smaller nuclei, two or three neutrons and gamma rays.
  • Chain reactions, controlled in a reactor and uncontrolled in a weapon; drawing them.
  • Fusion joins two light nuclei, converting some mass into energy.

4.5Forces

Paper 2

4.5.1Forces and their interactions

  • Scalars and vectors; forces as arrows.
  • Contact forces (friction, air resistance, tension, normal contact) and non-contact forces (gravitational, electrostatic, magnetic).
  • Weight, centre of mass, and weight in proportion to mass.
  • The resultant of forces along a line.
  • HT Free body diagrams; resolving a force into two components; scale vector diagrams for resultants and equilibrium.
  • \(W = mg\)

4.5.2Work done and energy transfer

  • A force does work when it moves an object; 1 J = 1 N m.
  • Work against friction raises the temperature.
  • \(W = Fs\)

4.5.3Forces and elasticity

  • Stretching, bending and compressing need more than one force; elastic against inelastic deformation.
  • Extension is proportional to force up to the limit of proportionality; linear and non-linear graphs.
  • Work done on a spring is stored as elastic potential energy.
  • \(F = ke\)
  • \(E_{\mathrm{e}} = \tfrac{1}{2}ke^2\)

Required practical 6 · force and extension

4.5.4Moments, levers and gears Physics only

  • The moment of a force about a pivot, using the perpendicular distance.
  • Balanced objects: clockwise moments equal anticlockwise moments.
  • How levers and gears pass on turning effects.
  • \(M = Fd\)

4.5.5Pressure in fluids Physics only

  • Fluid pressure acts at right angles to any surface.
  • HT Pressure in a liquid grows with depth and density; upthrust; floating and sinking.
  • The atmosphere thins with height, so atmospheric pressure falls with height.
  • \(p = \dfrac{F}{A}\)
  • \(p = h\rho g\) HT

4.5.6.1Describing motion

  • Distance and displacement, speed and velocity; typical speeds (walk 1.5, run 3, cycle 6, sound 330 m/s).
  • Speed from the gradient of a distance–time graph; acceleration from the gradient of a velocity–time graph.
  • HT Circular motion has constant speed but changing velocity; tangents to curved distance–time graphs; distance from the area under a velocity–time graph.
  • Free fall at about 9.8 m/s²; terminal velocity. Physics only Velocity–time graphs for terminal velocity, explained by the forces.
  • \(s = vt\)
  • \(a = \dfrac{\Delta v}{t}\)
  • \(v^2 - u^2 = 2as\)

4.5.6.2Newton’s laws

  • First law: velocity changes only if there is a resultant force. HT Inertia.
  • Second law: acceleration is proportional to resultant force and inversely proportional to mass. HT Inertial mass as \(\dfrac{\text{force}}{\text{acceleration}}\).
  • Estimating speeds, accelerations and forces for road vehicles.
  • Third law: interacting objects exert equal and opposite forces.
  • \(F = ma\)

Required practical 7 · force, mass and acceleration

4.5.6.3Forces and braking

  • \(\text{stopping distance} = \text{thinking distance} + \text{braking distance}\).
  • Reaction times of 0.2 to 0.9 s, lengthened by tiredness, drugs, alcohol and distractions; measuring them.
  • Road, weather, brakes and tyres affect braking distance; brakes do work that heats them; dangers of large decelerations.
  • Estimate how emergency stopping distance changes over typical speeds. Physics only Read graphs of stopping distance against speed for different vehicles.
  • HT Estimate braking forces for road vehicles.

4.5.7Momentum HT

  • Momentum is conserved in a closed system; describe and explain examples such as collisions.
  • Physics only Calculations for events such as collisions.
  • Physics only Force is the rate of change of momentum; air bags, seat belts, crash mats, helmets and soft playground surfaces.
  • \(p = mv\)
  • \(F = \dfrac{m\Delta v}{\Delta t}\) Physics only

4.6Waves

Paper 2

4.6.1Waves in air, fluids and solids

  • Transverse and longitudinal waves (compressions and rarefactions); the wave moves, not the medium.
  • Amplitude, wavelength, frequency and period; measuring the speed of sound and of ripples.
  • Physics only How speed, frequency and wavelength change when sound enters a new medium.
  • \(T = \dfrac{1}{f}\)
  • \(v = f\lambda\)

Required practical 8 · waves in a ripple tank and a solid

4.6.1.3–5Reflection, sound and ultrasound Physics only

  • Reflection, absorption and transmission at boundaries; ray diagrams for reflection.
  • HT Sound turned into vibrations of solids, as in the ear; the 20 Hz to 20 kHz hearing range.
  • HT Ultrasound imaging and echo sounding; P-waves and S-waves as evidence for the Earth’s core.

Required practical 9 Physics only · reflection and refraction of light

4.6.2Electromagnetic waves

  • The spectrum from radio to gamma; all at the same speed in a vacuum; transverse waves that transfer energy.
  • Ray diagrams for refraction. HT Wavefront diagrams; absorption, transmission, refraction and reflection depending on wavelength.
  • HT Radio waves made by, and inducing, oscillations in circuits.
  • Hazards of ultraviolet, X-rays and gamma rays; dose in sieverts.
  • Uses of each type. HT Why each type suits its use.

Required practical 10 · infrared from different surfaces

4.6.2.5–6Lenses and visible light Physics only

  • Convex and concave lenses, principal focus, focal length, real and virtual images, ray diagrams.
  • Specular and diffuse reflection; colour filters; why opaque objects have a colour; transparent and translucent.
  • \(\text{magnification} = \dfrac{\text{image height}}{\text{object height}}\)

4.6.3Black body radiation Physics only

  • Every object emits and absorbs infrared; hotter objects emit more, with a spread of wavelengths that depends on temperature.
  • A perfect black body absorbs everything and is the best emitter.
  • HT Temperature depends on the balance of absorbed and emitted radiation, including for the Earth.

4.7Magnetism and electromagnetism

Paper 2

4.7.1Magnets and magnetic fields

  • Poles; like poles repel, unlike attract; permanent and induced magnets.
  • Field lines run north to south and are densest at the poles; plotting them with a compass.
  • The Earth’s magnetic field as evidence of a magnetic core.

4.7.2The motor effect

  • The field around a wire and a solenoid; an iron core makes an electromagnet.
  • Physics only Explaining electromagnetic devices from diagrams.
  • HT Fleming’s left-hand rule; the force on a wire; how a coil turns in a motor.
  • Physics only HT Loudspeakers and headphones.
  • \(F = BIl\) HT

4.7.3Induced potential and transformers Physics only HT

  • The generator effect; the induced current opposes the change; factors affecting its size and direction.
  • Alternators (ac) and dynamos (dc), with graphs of p.d. against time; moving-coil microphones.
  • Transformers: primary and secondary coils on an iron core; step-up and step-down; power in equals power out at 100% efficiency; why the Grid transmits at high p.d.
  • \(\dfrac{V_{\mathrm{p}}}{V_{\mathrm{s}}} = \dfrac{n_{\mathrm{p}}}{n_{\mathrm{s}}}\)
  • \(V_{\mathrm{s}}I_{\mathrm{s}} = V_{\mathrm{p}}I_{\mathrm{p}}\)

4.8Space physics Physics only

Paper 2

4.8.1Solar system, stars and orbits

  • The Sun, eight planets, dwarf planets and moons, within the Milky Way.
  • A star forms from a nebula pulled together by gravity; fusion balances gravitational collapse.
  • Life cycles of a Sun-sized star and of a much more massive one; elements heavier than iron made in supernovae.
  • Gravity keeps planets and satellites in orbit. HT Changing velocity at constant speed; a change in speed needs a change in radius.

4.8.2Red-shift

  • Light from distant galaxies is red-shifted, more for those further away.
  • Evidence for an expanding universe and the Big Bang; since 1998, the expansion seems to be speeding up.
  • Dark mass and dark energy are still not understood.

3 Required practicals

Ten practicals that every student carries out. Exam questions on them carry at least 15% of the marks. Dashed boxes are physics only.

  1. 1
    Specific heat capacityEnergy · 4.1.1
  2. 2
    Thermal insulatorsEnergy · 4.1.2 · physics only
  3. 3
    ResistanceLength of a wire; resistors in series and parallel · 4.2.1
  4. 4
    I–V characteristicsFilament lamp, diode and fixed resistor · 4.2.1
  5. 5
    DensityRegular and irregular solids, and liquids · 4.3.1
  6. 6
    Force and extensionA spring · 4.5.3
  7. 7
    AccelerationVarying force, then varying mass · 4.5.6.2
  8. 8
    WavesRipple tank, and waves in a solid · 4.6.1
  9. 9
    LightReflection from surfaces, refraction by substances · 4.6.1.3 · physics only
  10. 10
    Infrared radiationAbsorption and emission by different surfaces · 4.6.2

4 Working scientifically and maths

Assessed in both papers, inside questions on any topic.

Working scientifically

  • How models and theories change with new evidence; using models; risk, ethics, applications and peer review.
  • Hypotheses, planning, independent, dependent and control variables, choosing apparatus, safety.
  • Tables, graphs, means, uncertainty, anomalies, conclusions and evaluation.
  • Scientific vocabulary, SI units, prefixes and significant figures.

Maths

  • Decimals, standard form, ratios, fractions, percentages and estimates.
  • Significant figures, means, charts, correlation and orders of magnitude.
  • The symbols \(=\), \(<\), \(>\), \(\propto\) and \(\sim\); rearranging and substituting into equations.
  • Plotting graphs, gradient and intercept, tangents to curves, and area under a graph.
  • Angles, 2D and 3D shapes, areas and volumes.