Key term
OCR A-Level Physics A H556
Practical Skills in the Written Papers
The Practical Endorsement
Topic overviewAnalogue and digital measuring instrumentsImproving accuracy with repeat timing, fiducial markers and plumb linesTiming, calipers and micrometersConstructing and testing circuitsSignal generators and oscilloscopesGenerating and measuring wavesData loggers, modelling software and ionising radiation
Physical Quantities and Units
Making Measurements and Analysing Data
Nature of Quantities
Motion
Forces in Action
Work, Energy and Power
Materials
Newton’s Laws of Motion and Momentum
Charge and Current
Energy, Power and Resistance
Electrical Circuits
Waves
Topic overviewProgressive waves and their propertiesThe wave equationReflection, refraction and diffractionWave graphs and intensityThe electromagnetic spectrumPolarisationRefraction and refractive indexCritical angle and total internal reflectionThe principle of superpositionInterference, coherence and path differenceTwo-source interference, Young's double-slit experiment and the diffraction gratingForming stationary wavesStationary waves on strings and in air columnsMeasuring the speed of soundNode spacing, amplitude and phase in stationary wavesHarmonics and the fundamental mode
Quantum Physics
Thermal Physics
Topic overviewThermal equilibrium and absolute temperatureThe kinetic model of solids, liquids and gasesBrownian motion and internal energySpecific heat capacityMeasuring specific heat capacitySpecific latent heatMeasuring specific latent heatMoles, the Avogadro constant and kinetic theoryGas laws, the ideal gas equation and r.m.s. speedMaxwell-Boltzmann distribution, Boltzmann constant and internal energy
Oscillations
Gravitational Fields
Astrophysics and Cosmology
Topic overviewThe solar system and the birth of a starThe death of a low-mass starSupernovae, neutron stars and black holesThe Hertzsprung-Russell diagramEnergy levels and emission spectraAbsorption spectra and spectral linesPhoton energy and the diffraction gratingWien's law and Stefan's lawAstronomical distances, parallax and the cosmological principleDoppler shift and Hubble's lawThe expanding universe and the Big BangEvidence for the Big Bang and dark energy
Capacitors
Topic overviewCapacitance and charging a capacitorCapacitors in seriesCapacitors in parallel and combined circuitsEnergy stored by a capacitorCharging and discharging through a resistorInvestigating capacitor dischargeThe time constantIterative modelling, exponential decay and the constant-ratio property
Electric Fields
Electromagnetism
Nuclear and Particle Physics
Topic overviewAlpha-particle scattering and the nuclear modelProton number, nucleon number and isotopesThe strong nuclear force and nuclear radiusParticles, antiparticles and hadronsLeptons and the quark modelQuark composition and chargesBeta decay in the quark modelRadioactive decay and the three radiationsNuclear decay equationsActivity, decay constant and half-lifeExponential decay and radioactive datingMass-energy equivalenceAnnihilation, mass defect and binding energyBinding energy per nucleon and induced fissionThe fission reactor and nuclear wasteNuclear fusion and balancing nuclear equations
Astrophysics and Cosmology
Wien's law and Stefan's law
- 2 things to know
- Papers 1, 2 and 3
Overview
Recall questions on Wien's displacement law, luminosity, Stefan's law and its calculations, and using Wien's law and Stefan's law together to estimate the radius of a star.
What you need to know
Answer each one before you reveal it.
Your recallNot started
Numbers
State Stefan's law and explain how luminosity depends on temperature.
Questions from this subtopic
Each one with the model answer underneath.
- 1
When estimating a star's radius from observations, how is Wien's displacement law used in the first step?
Model answer
Wien's law is used to determine the surface temperature from the peak wavelength of the star's emission spectrum.
- 2
State Wien's displacement law in words.
Model answer
The peak wavelength of emission from a black body is inversely proportional to its absolute temperature.
- 3
How can Wien's displacement law be used in stellar astronomy?
Model answer
It can be used to estimate the peak surface temperature of a star from its peak wavelength of emission.
- 4
Define luminosity of a star.
Model answer
Luminosity is the total power radiated by a star in all directions.
- 5
State Stefan's law and explain how luminosity depends on temperature.
Model answer
L = 4πr²σT⁴; luminosity is proportional to the surface area and the fourth power of the absolute surface temperature.
- 6
What does the symbol σ represent in Stefan's law?
Model answer
σ is the Stefan constant.
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