GCSE Physics

AQA GCSE · Combined 8464 · physics

Combined 8464.

The physics third of the double science GCSE on one page: its two exam papers, how the combined grade is awarded, then everything in the seven physics topics, with the equations and the eight physics required practicals.

An unofficial summary of the physics in the AQA GCSE Combined Science: Trilogy specification (8464, 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

Six written papers, two in each science, all sat at the end of the course at the same tier, Foundation or Higher. The table gives the two physics papers in full.

PaperTopicsTimeMarksWeight
Physics Paper 118 Energy, 19 Electricity, 20 Particle model of matter, 21 Atomic structure1 h 15 min7016.7%
Physics Paper 222 Forces, 23 Waves, 24 Magnetism and electromagnetism1 h 15 min7016.7%
Physics2 h 30 min14033.3%
Biology Papers 1 and 2, Chemistry Papers 1 and 2Topics 1–171 h 15 min each70 each16.7% each

Question types

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

Assessment objectives

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

The same split in every paper.

Practical skills

At least 15% of the marks come from questions on the 21 required practicals, eight of them in physics (listed below). 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)

2 How the grade is awarded

Combined 8464 gives one double grade for all three sciences. There is no separate physics grade.

420

One total

The raw marks of all six papers are added, each counting once (70 × 6 = 420). Grade boundaries are set on that total.

140

Physics share

The two physics papers are 140 of the 420 marks, a third of the grade, the same as biology and chemistry.

17

Point scale

Grades run from 1–1 to 9–9, the best. Each is a pair of equal or adjacent numbers, such as 6–6 or 6–5.

1

Series

The course is linear: all six papers are sat in the same May/June series.

The 17 grades and the tiers

  1. 9–9
  2. 9–8
  3. 8–8
  4. 8–7
  5. 7–7
  6. 7–6
  7. 6–6
  8. 6–5
  9. 5–5
  10. 5–4
  11. 4–4
  12. 4–3
  13. 3–3
  14. 3–2
  15. 2–2
  16. 2–1
  17. 1–1

Below the lowest grade of the tier the result is U (unclassified) and no certificate is given.

3 Physics subject content

Seven topics, in the specification’s order and numbering (section 6). They are the content of GCSE Physics without its physics-only parts (including all of Space physics), plus one Higher tier transformer equation.

6.1Energy

Physics Paper 1 · topic 18

6.1.1Energy 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 14 · specific heat capacity

6.1.2Conservation 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.
  • \(\text{efficiency} = \dfrac{\text{useful output energy}}{\text{total input energy}}\)
  • \(\text{efficiency} = \dfrac{\text{useful power output}}{\text{total power input}}\)

6.1.3National 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.

6.2Electricity

Physics Paper 1 · topic 19

6.2.1Current, 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 15 · resistance, and 16 · I–V characteristics

6.2.2Series 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)

6.2.3Domestic 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.

6.2.4Energy 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. How a transformer is built is not needed.
  • HT Use the transformer power equation from the equations sheet.
  • \(P = VI\)
  • \(P = I^2R\)
  • \(E = Pt\)
  • \(E = QV\)
  • \(V_{\mathrm{p}}I_{\mathrm{p}} = V_{\mathrm{s}}I_{\mathrm{s}}\) HT

6.3Particle model of matter

Physics Paper 1 · topic 20

6.3.1Changes 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 17 · density

6.3.2Internal 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.
  • \(\Delta E = mc\Delta\theta\)
  • \(E = mL\)

6.3.3Particle model and pressure

  • Gas molecules move randomly; temperature relates to their average kinetic energy.
  • At constant volume, a hotter gas exerts a higher pressure.

6.4Atomic structure

Physics Paper 1 · topic 21

6.4.1Atoms 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.

6.4.2Atoms 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.

6.5Forces

Physics Paper 2 · topic 22

6.5.1Forces 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.
  • \(W = mg\)

6.5.2Work done and energy transfer

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

6.5.3Forces 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 18 · force and extension

6.5.4.1Describing 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; an object falling through a fluid reaches terminal velocity.
  • \(s = vt\)
  • \(a = \dfrac{\Delta v}{t}\)
  • \(v^2 - u^2 = 2as\)

6.5.4.2Newton’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 19 · force, mass and acceleration

6.5.4.3Forces and braking

  • \(\text{stopping distance} = \text{thinking distance} + \text{braking distance}\); faster means further for a given braking force.
  • 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.
  • HT Estimate braking forces for road vehicles.

6.5.5Momentum HT

  • Momentum as mass × velocity.
  • Momentum is conserved in a closed system; describe and explain examples such as collisions.
  • \(p = mv\)

6.6Waves

Physics Paper 2 · topic 23

6.6.1Waves 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.
  • \(T = \dfrac{1}{f}\)
  • \(v = f\lambda\)

Required practical 20 · waves in a ripple tank and a solid

6.6.2Electromagnetic 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 21 · infrared from different surfaces

6.7Magnetism and electromagnetism

Physics Paper 2 · topic 24

6.7.1Magnets 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.

6.7.2The motor effect

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

4 Physics required practicals

Eight of the course’s 21 required practicals are physics, numbered 14 to 21. Biology and chemistry have the rest.

  1. 14
    Specific heat capacityEnergy · 6.1.1
  2. 15
    ResistanceLength of a wire; resistors in series and parallel · 6.2.1
  3. 16
    I–V characteristicsFilament lamp, diode and fixed resistor · 6.2.1
  4. 17
    DensityRegular and irregular solids, and liquids · 6.3.1
  5. 18
    Force and extensionA spring · 6.5.3
  6. 19
    AccelerationVarying force, then varying mass · 6.5.4.2
  7. 20
    WavesRipple tank, and waves in a solid · 6.6.1
  8. 21
    Infrared radiationAbsorption and emission by different surfaces · 6.6.2

5 Working scientifically and maths

Assessed in every paper, 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.