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AQA A-level Physics data and formulae sheet (7408): what is on it and what is not

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Formula sheet

The card below opens today's A-level Physics paper with this sheet in the drawer, so you practise the way you will sit the exam. The contents follow, grouped like the real booklet in our own layout and words. Check against AQA's Physics data and formulae before you rely on anything here.

Formula sheet

A-level Physics: Year 1

Open formula sheet

Fundamental constants and values

QuantitySymbolValueUnit
speed of light in a vacuumc3.00 × 10⁸m s⁻¹
permeability of free spaceμ₀4π × 10⁻⁷H m⁻¹
permittivity of free spaceε₀8.85 × 10⁻¹²F m⁻¹
magnitude of the charge of an electrone1.60 × 10⁻¹⁹C
the Planck constanth6.63 × 10⁻³⁴J s
gravitational constantG6.67 × 10⁻¹¹N m² kg⁻²
the Avogadro constantNA6.02 × 10²³mol⁻¹
molar gas constantR8.31J K⁻¹ mol⁻¹
the Boltzmann constantk1.38 × 10⁻²³J K⁻¹
the Stefan constantσ5.67 × 10⁻⁸W m⁻² K⁻⁴
the Wien constantα2.90 × 10⁻³m K
electron rest massmₑ9.11 × 10⁻³¹kg
electron charge to mass ratioe/mₑ1.76 × 10¹¹C kg⁻¹
proton rest massmₚ1.673 × 10⁻²⁷kg
proton charge to mass ratioe/mₚ9.58 × 10⁷C kg⁻¹
neutron rest massmₙ1.675 × 10⁻²⁷kg
gravitational field strengthg9.81N kg⁻¹
acceleration due to gravityg9.81m s⁻²
atomic mass unitu1.661 × 10⁻²⁷kg

Astronomical data

BodyMass / kgMean radius / m
Sun1.99 × 10³⁰6.96 × 10⁸
Earth5.97 × 10²⁴6.37 × 10⁶

Photons and energy levels

E=hf=\frac{hc}{\lambda}photon energy
hf=\phi+E_{k(max)}photoelectric equation
hf=E_1-E_2energy levels
\lambda=\frac{h}{p}de Broglie wavelength

Waves

v=f\lambdawave speed
f=\frac{1}{T}frequency and period
f=\frac{1}{2l}\sqrt{\frac{T}{\mu}}first harmonic on a string
w=\frac{\lambda D}{s}double slit fringe spacing
d\sin\theta=n\lambdadiffraction grating
n=\frac{c}{v}refractive index
n_1\sin\theta_1=n_2\sin\theta_2law of refraction
\sin C=\frac{n_2}{n_1}critical angle (n₁ > n₂)

Mechanics

\text{moment}=Fxmoment
v=u+atfinal velocity
s=\frac{1}{2}(u+v)tdisplacement from the average velocity
v^2=u^2+2asvelocity without time
s=ut+\frac{1}{2}at^2displacement from the start velocity
F=maresultant force
F=\frac{\Delta p}{\Delta t}force as the rate of change of momentum
F\Delta t=\Delta pimpulse
W=Fs\cos\thetawork done
E_k=\frac{1}{2}mv^2kinetic energy
\Delta E_p=mg\Delta hchange in gravitational potential energy
P=\frac{W}{t}power
P=Fvpower from force and velocity
\text{efficiency}=\frac{\text{useful output}}{\text{total input}}efficiency

Materials

\rho=\frac{m}{V}density
F=kxHooke's law
E=\frac{\sigma}{\varepsilon}Young modulus
\sigma=\frac{F}{A}tensile stress
\varepsilon=\frac{\Delta L}{L}tensile strain
E=\frac{1}{2}F\Delta Lenergy stored in a stretched material

Electricity

I=\frac{\Delta Q}{\Delta t}current
V=\frac{W}{Q}potential difference
R=\frac{V}{I}resistance
R=\frac{\rho L}{A}resistivity
R_T=R_1+R_2+R_3+\cdotsresistors in series
\frac{1}{R_T}=\frac{1}{R_1}+\frac{1}{R_2}+\frac{1}{R_3}+\cdotsresistors in parallel
P=VI=I^2R=\frac{V^2}{R}electrical power
\varepsilon=\frac{E}{Q}emf
\varepsilon=I(R+r)emf and internal resistance

Circular motion

\omega=\frac{2\pi}{T}=2\pi fangular speed
a=\frac{v^2}{r}=\omega^2rcentripetal acceleration
F=\frac{mv^2}{r}=m\omega^2rcentripetal force

Simple harmonic motion

a=-\omega^2xacceleration in simple harmonic motion
x=A\cos\omega tdisplacement in simple harmonic motion
v=\pm\omega\sqrt{A^2-x^2}speed in simple harmonic motion
v_{max}=\omega Amaximum speed
a_{max}=\omega^2Amaximum acceleration
T=2\pi\sqrt{\frac{m}{k}}period of a mass on a spring
T=2\pi\sqrt{\frac{l}{g}}period of a simple pendulum

Thermal physics

Q=mc\Delta\thetaenergy to change temperature
Q=mlenergy to change state
pV=nRTideal gas equation, moles
pV=NkTideal gas equation, molecules
pV=\frac{1}{3}Nm\overline{c^2}kinetic theory of gases
\frac{1}{2}m\overline{c^2}=\frac{3}{2}kT=\frac{3RT}{2N_A}mean kinetic energy of a gas molecule

Gravitational fields

F=\frac{Gm_1m_2}{r^2}gravitational force between two masses
g=\frac{F}{m}gravitational field strength
g=\frac{GM}{r^2}gravitational field strength of a point mass
\Delta W=m\Delta Vwork done in a gravitational field
V=-\frac{GM}{r}gravitational potential
g=-\frac{\Delta V}{\Delta r}field strength from potential

Electric fields and capacitors

F=\frac{Q_1Q_2}{4\pi\varepsilon_0r^2}force between two point charges
F=EQforce on a charge
E=\frac{V}{d}uniform electric field
E=\frac{Q}{4\pi\varepsilon_0r^2}electric field of a point charge
V=\frac{Q}{4\pi\varepsilon_0r}electric potential of a point charge
C=\frac{Q}{V}capacitance
C=\frac{A\varepsilon_0\varepsilon_r}{d}parallel plate capacitor
E=\frac{1}{2}QV=\frac{1}{2}CV^2=\frac{Q^2}{2C}energy stored in a capacitor
Q=Q_0\left(1-e^{-t/RC}\right)capacitor charging
Q=Q_0e^{-t/RC}capacitor discharge
RCtime constant

Magnetic fields

F=BIlforce on a current
F=BQvforce on a moving charge
\Phi=BAmagnetic flux
N\Phi=BAN\cos\thetaflux linkage
\varepsilon=-N\frac{\Delta\Phi}{\Delta t}induced emf
\varepsilon=BAN\omega\sin\omega temf induced in a rotating coil
I_{rms}=\frac{I_0}{\sqrt{2}},\quad V_{rms}=\frac{V_0}{\sqrt{2}}root mean square values
\frac{N_s}{N_p}=\frac{V_s}{V_p}transformer
\text{efficiency}=\frac{I_sV_s}{I_pV_p}transformer efficiency

Nuclear physics

I=\frac{k}{x^2}inverse square law for gamma radiation
\frac{\Delta N}{\Delta t}=-\lambda N,\quad N=N_0e^{-\lambda t}radioactive decay
A=\lambda Nactivity
T_{1/2}=\frac{\ln2}{\lambda}half-life
R=R_0A^{1/3}nuclear radius
E=mc^2energy-mass equation

Option topics

The booklet closes with data and equations for the five option topics, all of them in the drawer, summarised here by topic.

OptionWhat it gives
Astrophysicsastronomical unit, light year, parsec, Hubble constant, telescope, Rayleigh criterion, magnitude, Wien and Stefan laws, Schwarzschild radius, Doppler shift and red shift
Medical physicslens equations, threshold of hearing, intensity level, absorption and ultrasound impedance, effective half-life
Engineering physicsmoment of inertia, angular kinetic energy and motion, torque, thermodynamics, heat engines, heat pumps
Turning points in physicselectrons in fields, Millikan, Maxwell's formula, de Broglie, special relativity
Electronicsresonant frequency, Q-factor, operational amplifiers, bandwidth for AM and FM

Gaps in the AQA booklet

  • No equation for current in a conductor (I = nAvq), no pressure equation and no Stokes' law. They come from your own revision.
  • No definitions and no units next to the equations. The constants carry units; the equations do not.
  • Option equations for topics you did not study. The last pages cover all five options, but you answer only the one you were taught.

Working with the 7408 booklet

Version 1.5 opens with a table of fundamental constants and the astronomical data for the Sun and Earth, followed by the particle physics tables and then the equations by topic. Learn that order: constants, particle tables, then photons, waves, mechanics and on through the course.

Note that g appears twice, as 9.81 N kg⁻¹ and as 9.81 m s⁻². Both are on the sheet, so use whichever matches the units in your working.

Work out a photon energy from its frequency or wavelength, in units of 10^-19 J.

Press Mark to have your answer marked in the Light & Energy course.

Worked example: the photoelectric effect

Light of frequency 1.2 × 10¹⁵ Hz falls on a metal with a work function of 4.0 × 10⁻¹⁹ J. Find the maximum kinetic energy of the electrons, using h from the booklet.

E_{k(max)}=hf-\phi=(6.63\times10^{-34})(1.2\times10^{15})-4.0\times10^{-19}=3.96\times10^{-19}\ \text{J}

The photon carries 7.96 × 10⁻¹⁹ J and the electron keeps about half. The usual slip is to quote hf as the answer.

The AQA sheet and the other boards

BoardSheetWhat it holds
AQA (this guide)A-level Physics data and formulae (7408), version 1.5Constants and astronomical data, equations by topic, then five option sections
EdexcelList of data, formulae and relationships (9PH0), Issue 3, November 2022Fourteen data values, then equations in twelve sections from Mechanics to Oscillations
OCR AData, Formulae and Relationships Booklet (H156, H556), 8 pagesConstants, conversion factors and maths equations, then equations by module; no kinetic energy line
EduqasData Booklet, A level component 3 (2019 paper)Values and conversions, one list of equations, options A to D, and maths information
WJECData Booklet, A2 unit 3 (2019 paper)The same layout as Eduqas, without the option sections
CCEAData and formulae sheet for A2 Units 1 and 2 (APH11, APH21)Constants and a short list of "useful formulae"; the Hubble constant is given as about 2.4 × 10⁻¹⁸ s⁻¹

AQA's is the only sheet here with an astronomical data table and with five option sections: astrophysics, medical physics, engineering physics, turning points and electronics. Edexcel and OCR print no options.

Exam answers

You will find our own worked answers after marking a daily paper. They are written for this site and are not AQA's.

Daily papers to try with the AQA sheet

Both daily tracks, A-level Physics 1 and Physics 2, are 8-question papers. They are far shorter than a 7408 paper, so expect to finish quickly and spend the spare minutes checking which booklet entry you used.

Slips with the AQA booklet

  • Using the astronomical data from memory instead of the table.
  • Reading a radioactive decay line without noticing it has two forms.
  • Taking F = BIl as the full force when the angle is not 90°.

Common questions

Do you get a data sheet in AQA A-level Physics?
Yes. AQA publishes A-level Physics data and formulae for use in exams from the June 2017 series onwards.
What is in the AQA A-level Physics data and formulae booklet?
Fundamental constants, astronomical data, particle physics tables, equations for each topic, and data and equations for the optional topics.
Does the AQA booklet define the symbols?
No. It prints equations and data, so you need to know what each symbol means.
What is not on the AQA data sheet?
Definitions, units for the equations, derivations, and some equations such as current in a conductor and Stokes' law.
Is the AQA physics data sheet the same as Edexcel or OCR?
No. Each board prints its own, with different constants, layouts and equations.

Revision cards

Say the answer first, then flip the card to check it.

Where to go next

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  • Test it

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