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Scheme of work · Cambridge International AS and A Level Physics 9702

A Level Physics scheme of work

77 lessons in 25 topics, in syllabus order: 57 hours 45 minutes of teaching at 45 minutes a lesson. Set your lessons per week and the week numbers follow. Every lesson links to its pack, every topic to its lab, question bank and notes.

Lesson packs
26 weeks for the course at 3 a weekRemembered in this browser.
At a glance

The course in numbers

Lessons
77, one 45-minute lesson pack each
Teaching time
57 hours 45 minutes
Weeks
26 at 3 lessons a week
AS Level
11 topics, 34 lessons, 25 hours 30 minutes
A Level (A2)
14 topics, 43 lessons, 32 hours 15 minutes
Assessment points
11 topic question banks, assignable in the app
Labs
24 full-screen topic labs to project

How to read it. One row is one 45-minute lesson; its pack holds the plan, worksheet and quiz. The week column counts 3 lessons a week until you change the control above; the sheet you download uses the same numbers. Each topic ends at an assessment point, its question bank, which you can assign in the app for a marked score. The learning intention is the first idea of each lesson in the students' own pages; the traps are the examiner traps those pages pre-empt.

AS Level

Year 1: the AS topics

Weeks 1 to 12

Topic 1Physical quantities and units

Week 1
WeekRefLessonLearning intention
11.1-1.2Physical quantities and unitsReduce each side of an equation to SI base units and put them on a balance.
11.3Errors and uncertaintiesThe bullseye is the true value.
11.4Scalars and vectorsSet two vectors and watch their resultant form nose to tail, with its perpendicular components drawn in.
1Assessment pointTopic question bank, 53 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Do not treat a successful homogeneity check as proof.
  • Do not claim that "taking more readings improves accuracy".
  • Do not add vectors by adding their magnitudes.

2.1Kinematics

Week 2
WeekRefLessonLearning intention
22.1Linear motion and graphsSet an initial velocity and an acceleration, then run the trolley.
22.1Equations of motionDrop a ball from rest.
22.1Projectile motionSet a launch speed and angle and fire.
2Assessment pointTopic question bank, 51 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Match the operation to the right graph.
  • Two slips cost marks here.
  • Never mix the components.

Topic 3Dynamics

Week 3
WeekRefLessonLearning intention
33.1Newton's laws and momentumA constant force pushes a cart on a frictionless track.
33.2Motion with resistanceDrop an object and watch the two arrows.
33.3Conservation of momentumSet the masses and velocities of two trolleys and choose elastic or inelastic.
3Assessment pointTopic question bank, 51 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • The classic error is to pair the weight of an object with the normal contact force from the surface it rests on.
  • Terminal velocity is a constant velocity, which means the acceleration is zero, not that there are no forces.
  • Two traps recur.

Topic 4Forces, density and pressure

Week 4
WeekRefLessonLearning intention
44.1Turning effects of forcesSlide the loads along the beam and change their weights.
44.2Equilibrium of forcesA weight hangs from two strings.
44.3Density and pressureLower a 1 litre block into the liquid and change the two densities.
4Assessment pointTopic question bank, 51 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Use the perpendicular distance, not the distance along the force or the slanted distance to the pivot.
  • Equilibrium needs both conditions.
  • Liquid pressure depends on depth and density only, never on the shape of the container or the area of its base; a narrow tube and a wide tank filled to the same depth have the same pressure at the bottom.

Topic 5Work, energy and power

Week 5
WeekRefLessonLearning intention
55.1Work, energy and powerA constant force drags a crate at a steady speed against friction.
55.2Kinetic and potential energyRelease the ball and watch the two energy bars trade: gravitational potential energy falls as kinetic energy rises, while the total stays fixed.
5Assessment pointTopic question bank, 40 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Two slips recur.
  • Kinetic energy depends on v², not v, so doubling the speed quadruples the kinetic energy (and the braking distance).

Topic 6Deformation of solids

Weeks 5 to 6
WeekRefLessonLearning intention
56.1Stress, strain and the Young modulusAdd load to the wire and trace the force-extension graph.
66.2Elastic potential energyStretch the spring and watch the shaded triangle under the force-extension line grow.
6Assessment pointTopic question bank, 38 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Keep the limits straight: the limit of proportionality is where the graph stops being straight, while the elastic limit is where permanent deformation begins; they are close but not the same.
  • The stored energy is the triangle area ½Fx, not Fx; using the full rectangle doubles the answer.

Topic 7Waves

Weeks 6 to 7
WeekRefLessonLearning intention
67.1Progressive wavesAdjust the frequency and wavelength and watch the wave travel; the read-out confirms v = fλ at every setting.
67.2Transverse and longitudinal wavesSwitch between transverse and longitudinal and watch how the particles move relative to the energy travel.
77.3The Doppler effectMove the source and watch the circular wavefronts crowd together in front and spread out behind.
77.4The electromagnetic spectrumMove along the spectrum and watch the wavelength and frequency trade off through c = fλ, with the named regions and the narrow visible band highlighted.
77.5PolarisationRotate the second polariser and watch the transmitted intensity follow I = I₀ cos²θ: bright when aligned, dark when crossed at 90°.
7Assessment pointTopic question bank, 40 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Keep amplitude and intensity distinct: intensity goes as amplitude squared, so halving the amplitude quarters the intensity.
  • Do not confuse the graph shape with the motion.
  • Get the sign right: subtract the source speed in the denominator for an approaching source (which raises the frequency) and add it for a receding one.

Topic 8Superposition

Weeks 8 to 9
WeekRefLessonLearning intention
88.1Stationary wavesStep through the harmonics of a string fixed at both ends and watch nodes stay still while antinodes oscillate.
88.2DiffractionChange the gap width relative to the wavelength and watch the diffracted wavefronts spread.
88.3InterferenceChange the slit separation, the wavelength and the screen distance and watch the fringe pattern respond exactly as λ = ax / D predicts.
98.4The diffraction gratingSet the wavelength and the grating spacing and watch the orders appear at the angles given by d sinθ = nλ, with the highest visible order limited by sinθ ≤ 1.
9Assessment pointTopic question bank, 48 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Adjacent nodes are half a wavelength apart, not a whole wavelength, so the wavelength is twice the node spacing.
  • Diffraction does not change the wavelength, frequency or speed of the wave; it only changes its direction of spread.
  • The two sources must be coherent; two ordinary lamps will not interfere because their phase difference is random.

Topic 9Electricity

Weeks 9 to 10
WeekRefLessonLearning intention
99.1Electric currentWatch the charge carriers drift along the conductor.
99.2Potential difference and powerSet the voltage across a resistor and the current follows from V = IR; watch the power dissipated track P = VI and the three equivalent forms agree at every setting.
109.3Resistance and resistivitySweep the voltage and plot the I-V characteristic for a metal conductor, a filament lamp and a diode, and see why only the first is a straight line through the origin.
10Assessment pointTopic question bank, 42 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Keep the symbols in I = Anvq straight: n is the number of carriers per unit volume, not the total number in the wire.
  • The three power formulas are equivalent, not different physics: pick the one matching your known quantities.
  • Resistance R = V/I is the value at a point, found from the coordinates, not the gradient, on a curved I-V graph.

Topic 10D.C. circuits

Weeks 10 to 11
WeekRefLessonLearning intention
1010.1E.M.F. and internal resistanceDraw more current from the cell and watch the terminal voltage fall below the e.m.f. by the lost volts Ir.
1010.2Kirchhoff lawsSwitch resistors between series and parallel and watch the currents split and recombine while the totals obey both Kirchhoff laws and the combination rules.
1110.3Potential dividersMove the divider tap, or swap in a thermistor or LDR, and watch the output voltage follow V × R₂ / (R₁ + R₂) as the resistances change.
11Assessment pointTopic question bank, 42 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • The e.m.f. is not simply the voltage you read across a battery in use; that is the terminal p.d., which is lower by Ir.
  • Add resistances directly only in series; in parallel you must add the reciprocals, and the result is always less than the smallest branch.
  • Use the resistance of the component you take the output across in the numerator: Vₒᵤₜ = V R₂/(R₁ + R₂).

Topic 11Particle physics

Weeks 11 to 12
WeekRefLessonLearning intention
1111.1The atom and radiationFire alpha particles past a nucleus and vary the aim.
1111.1Antiparticles and neutrinosWatch a neutron decay: an electron and an antineutrino fly out, sharing the available energy.
1211.2Quarks and leptonsCombine up and down quarks and read off the total charge.
12Assessment pointTopic question bank, 42 multiple-choice questions: print or review, or assign in the app for a marked score.
Examiner traps to pre-empt:
  • Most alpha particles pass straight through the foil because the atom is mostly empty space; only a near head-on approach to the tiny nucleus gives a large deflection.
  • An antiparticle has the same mass as its particle, only the charge is reversed; do not say it is lighter or heavier.
  • Quark charges are fractional: up is +2/3 e and down is −1/3 e, and they add to give the whole-number charge of the particle.
A Level (A2)

Year 2: the A2 topics

Weeks 12 to 26

Topic 12Motion in a circle

Week 12
2 lessons, 1 hour 30 minutesTopic planLab: Circular motionNotes PDF
WeekRefLessonLearning intention
1212.1Angular quantitiesA point on a spinning disc sweeps out equal angles in equal times.
1212.2Centripetal acceleration and forceSwing a ball on a string in a vertical circle.

Topic 13Gravitational fields

Week 13
WeekRefLessonLearning intention
1313.1-13.2Gravitational field and Newton's lawA mass placed near a planet feels a pull even with nothing touching it.
1313.2-13.3Orbits and field strengthA satellite in a circular orbit has only one force on it: the planet's gravity, and that single force is the centripetal force.
1313.4Gravitational potentialGravitational potential is the work done per kilogram to bring a mass from infinity to a point.

Topic 14Temperature

Week 14
3 lessons, 2 hours 15 minutesTopic planLab: TemperatureNotes PDF
WeekRefLessonLearning intention
1414.1Thermal equilibriumBring a hot object and a cold one together and energy crosses the boundary from hot to cold.
1414.2Temperature scalesMany properties change with temperature, but two thermometers using different properties need not agree between their fixed points.
1414.3Specific heat and latent heatSupply energy at a steady rate and the temperature climbs on the sloping parts and holds steady on the flat parts.

Topic 15Ideal gases

Week 15
3 lessons, 2 hours 15 minutesTopic planLab: Ideal gasesNotes PDF
WeekRefLessonLearning intention
1515.1The moleAtoms and molecules come in numbers far too large to count one by one, so we group them: one mole is a fixed, enormous number of particles, the Avogadro number.
1515.2The equation of stateFor a fixed amount of ideal gas the three quantities are tied by one relation.
1515.3Kinetic theory of gasesPressure is not a property of single molecules; it is the steady drumbeat of countless collisions on the walls.

Topic 16Thermodynamics

Week 16
2 lessons, 1 hour 30 minutesTopic planLab: ThermodynamicsNotes PDF
WeekRefLessonLearning intention
1616.1Internal energyInternal energy is not the heat in a body or its temperature; it is the grand total of the random kinetic and potential energies of every molecule.
1616.2The first law of thermodynamicsWhen a gas expands at constant pressure it pushes a piston back, doing work W = pΔV.

Topic 17Oscillations

Weeks 16 to 17
3 lessons, 2 hours 15 minutesTopic planLab: OscillationsNotes PDF
WeekRefLessonLearning intention
1617.1Simple harmonic motionSet an oscillation going and three curves emerge together.
1717.2Energy in simple harmonic motionAs an oscillator moves, energy sloshes between kinetic and potential.
1717.3Damping and resonanceA real oscillator loses energy to resistive forces and its amplitude decays: it is damped.

Topic 18Electric fields

Weeks 17 to 19
5 lessons, 3 hours 45 minutesTopic planLab: Electric fieldsNotes PDF
WeekRefLessonLearning intention
1718.1Electric fields and field linesSwitch between a single charge, a dipole, like charges and parallel plates.
1818.2Uniform electric fieldsSet the plate voltage and separation to control E = V/d, then watch a positive charge curve toward the negative plate.
1818.3Coulomb’s lawVary the two charges and their separation.
1818.4Electric field of a point chargeField lines stream straight out from a positive charge or straight in to a negative one.
1918.5Electric potentialCompare the 1/r potential with the 1/r² field for the same point charge.

Topic 19Capacitance

Weeks 19 to 20
3 lessons, 2 hours 15 minutesTopic planLab: CapacitanceNotes PDF
WeekRefLessonLearning intention
1919.1Capacitors and capacitanceSwitch between a single capacitor and series or parallel pairs.
1919.2Energy stored in a capacitorVary C and V and watch the shaded triangle under the V-Q line.
2019.3Discharging a capacitorAdjust R and C to change the time constant and watch the curve stretch or steepen.

Topic 20Magnetic fields

Weeks 20 to 21
5 lessons, 3 hours 45 minutesTopic planLab: Magnetic fieldsNotes PDF
WeekRefLessonLearning intention
2020.1Magnetic fields and field linesSwitch the source between a bar magnet, a straight wire and a solenoid.
2020.2Force on a current-carrying conductorVary the flux density B, the current I, the length L in the field and the angle θ.
2120.3Force on a moving chargeIn the magnetic field, the force points to the centre and the charge loops round; change the speed or the field and watch the radius follow r = mv / BQ.
2120.4Magnetic fields due to currentsChoose the direction and size of each current and the separation.
2120.5Electromagnetic inductionAs the magnet moves through the coil the flux linkage rises and falls, and the e.m.f. follows its rate of change, reversing as the magnet leaves instead of enters.
Examiner traps to pre-empt:
  • Field lines never cross, because the field has a single direction at each point.
  • The angle factor is sinθ, not cosθ, and θ is between the current and the field: the force is a maximum when they are perpendicular and zero when parallel.
  • The magnetic force does no work: it changes direction, not speed, so the path is a circle, not a spiral that speeds up.

Topic 21Alternating currents

Week 22
WeekRefLessonLearning intention
2221.1Characteristics of alternating currentThe top trace is the current, i = I₀ sinωt.
2221.2Rectification and smoothingSwitch between half-wave and full-wave rectification and watch the output.
Examiner traps to pre-empt:
  • The simple average of a sinusoidal current over a whole cycle is zero, which is why we use the r.m.s. value instead.
  • The smoothing capacitor goes in parallel with the load, not in series.

Topic 22Quantum physics

Weeks 22 to 23
WeekRefLessonLearning intention
2222.1Energy and momentum of a photonSlide through the spectrum and watch the energy, frequency and momentum move together.
2322.2The photoelectric effectPick a metal, then lower the wavelength until electrons just begin to escape.
2322.3Wave-particle dualityFire electrons through a thin graphite film and they form diffraction rings.
2322.4Energy levels and line spectraChoose two hydrogen levels and watch the photon.
Examiner traps to pre-empt:
  • A photon's energy is set by its frequency, not by the brightness of the light.
  • Wave theory predicts that any frequency should eventually free electrons if you wait or brighten the light.
  • Everyday objects also have a de Broglie wavelength, but it is fantastically small (because their momentum is huge), so they never show diffraction.

Topic 23Nuclear physics

Week 24
2 lessons, 1 hour 30 minutesTopic planLab: Nuclear physicsNotes PDF
WeekRefLessonLearning intention
2423.1Mass defect and binding energySlide along the binding-energy-per-nucleon curve.
2423.2Radioactive decayEach nucleus winks out at random, but watch the count: with a whole sample it halves in a fixed half-life and traces the exponential, whatever half-life you choose.
Examiner traps to pre-empt:
  • Stability is measured by binding energy per nucleon, not total binding energy (uranium has the largest total but is far less stable than iron).
  • Activity and count rate fall on the same exponential as N, because both are proportional to N.

Topic 24Medical physics

Weeks 24 to 25
3 lessons, 2 hours 15 minutesTopic planLab: Medical physicsNotes PDF
WeekRefLessonLearning intention
2424.1Production and use of ultrasoundSet the acoustic impedance of two media and watch how much of the pulse echoes back.
2524.2Production and use of X-raysChoose a material and a thickness and watch the transmitted intensity fall along I = I₀e⁻μᵛ.
2524.3PET scanningEach annihilation sends two gamma photons to opposite detectors; the line joining them runs through the tracer.
Examiner traps to pre-empt:
  • The reflection coefficient depends on the difference in impedance, not the impedance itself; matched media (small Z₁ − Z₂) give almost no echo.
  • Only a small fraction of the electrons' energy becomes X-rays, the rest is heat, which is why the target must be cooled (often a rotating anode).
  • The 0.511 MeV photon energy is exactly the rest energy of an electron, m₋c²; two are produced so the total comes from the electron and the positron.

Topic 25Astronomy and cosmology

Weeks 25 to 26
WeekRefLessonLearning intention
2525.1Standard candles and the inverse square lawSet the distance and the luminosity, and watch the received flux fall away.
2625.2Stellar radii: Wien and Stefan-BoltzmannDrag the temperature and watch the black-body curve: its peak slides to shorter wavelengths as the star heats up, exactly as Wien's law demands, while the whole curve climbs because the power per unit area grows as T⁴.
2625.3Hubble's law and the Big BangSet a galaxy's distance and watch its spectral line slide into the red while the point climbs the straight v = H₀d line.
Examiner traps to pre-empt:
  • Keep luminosity (emitted, intrinsic, in W) apart from radiant flux intensity (received, in W m⁻²).
  • In Wien's law λₘₐₓ is inversely proportional to T: a hotter star has a shorter peak wavelength, not a longer one.
  • A redshift is a shift to longer wavelength and lower frequency.
Also for this course

Beyond the scheme

Original work by the TheLucidSTEM team. Week numbers assume 3 lessons a week unless you change the control; the download carries the numbers shown.