Physics 0625 · for examination in 2026, 2027 and 2028
Formula list
Every equation named in the Cambridge IGCSE Physics syllabus, in the syllabus's own order, with the Core and Supplement split drawn where the syllabus draws it.
Compiled by GioPhysics from the published syllabus. This is an independent study aid, not a Cambridge document; the official syllabus is the authority. Check anything against the Cambridge IGCSE Physics 0625 syllabus before an exam.
Your route
Showing all 68 equations — 29 Core and 39 Supp.. The wider route is the narrower one plus the extension, so it covers every row on this page.
Download the whole list as a PDF Or take one topic at a time — every topic below has its own printable sheet. The PDFs are typeset from this same list, so they cannot say anything different from the page.
Motion, forces and energy
PDF1.1Physical quantities and measurement techniques
Resultant of two vectors at right angles
R = √(x² + y²)
- R
- resultant of the two vectors
- x, y
- the two perpendicular components
Forces or velocities only. A scale drawing is an accepted method — the syllabus asks for the resultant by calculation or graphically.
1.2Motion
Speed
v = s / t
Rearrangeds = vt · t = s / v
- v
- speedm/s
- s
- distance travelledm
- t
- time takens
Average speed
average speed = total distance travelled / total time taken
- distance
- the whole journeym
- time
- the whole journeys
Speed from a distance–time graph
speed = gradient of a distance–time graph
- gradient
- rise ÷ run of a straight-line section
Distance from a speed–time graph
distance travelled = area under a speed–time graph
- area
- of the region between the line and the time axis
For motion at constant speed or constant acceleration.
Acceleration
a = Δv / t
RearrangedΔv = at
- a
- accelerationm/s²
- Δv
- change in velocitym/s
- t
- time takens
A deceleration is a negative acceleration, and is used as such in calculations.
Acceleration from a speed–time graph
acceleration = gradient of a speed–time graph
- gradient
- rise ÷ run
1.3Mass and weight
Gravitational field strength
g = W / m
RearrangedW = mg · m = W / g
- g
- gravitational field strengthN/kg
- W
- weightN
- m
- masskg
The syllabus asks you to know that g is equivalent to the acceleration of free fall.
1.4Density
Density
ρ = m / V
Rearrangedm = ρV · V = m / ρ
- ρ
- densityg/cm³, kg/m³
- m
- masskg, g
- V
- volumem³, cm³
1.5.1Effects of forces
Resultant force and acceleration
F = ma
Rearrangeda = F / m · m = F / a
- F
- resultant forceN
- m
- masskg
- a
- accelerationm/s²
The force and the acceleration are in the same direction. F = mv²/r is explicitly not required at 0625.
Spring constant
k = F / x
RearrangedF = kx · x = F / k
- k
- spring constantN/m, N/cm
- F
- force (load)N
- x
- extensionm, cm
Valid up to the limit of proportionality. An understanding of the elastic limit is not required.
1.5.2Turning effect of forces
Moment of a force
moment = F × d
- F
- forceN
- d
- perpendicular distance from the pivotm
- moment
- turning effectN m
Principle of moments
sum of clockwise moments = sum of anticlockwise moments
- about
- the same pivot, for an object in equilibrium
Core covers one force each side of the pivot; Supplement extends it to more than one force each side.
1.5.3Centre of gravity
No equations. This point is examined through experiment and qualitative reasoning about stability.
1.6Momentum
Momentum
p = mv
Rearrangedm = p / v · v = p / m
- p
- momentumkg m/s, N s
- m
- masskg
- v
- velocitym/s
Impulse
impulse = FΔt = Δ(mv)
- F
- forceN
- Δt
- time for which the force actss
- Δ(mv)
- change in momentumkg m/s, N s
Resultant force from momentum
F = Δp / Δt
- F
- resultant forceN
- Δp
- change in momentumkg m/s
- Δt
- time takens
Conservation of momentum
total momentum before = total momentum after
- p
- summed for every object, with direction
Simple problems in one dimension only.
1.7.1Energy
Kinetic energy
Ek = ½mv²
Rearrangedv = √(2Ek / m)
- Ek
- kinetic energyJ
- m
- masskg
- v
- speedm/s
Change in gravitational potential energy
ΔEp = mgΔh
- ΔEp
- change in g.p.e.J
- m
- masskg
- g
- gravitational field strengthN/kg
- Δh
- change in heightm
Conservation of energy
total energy before = total energy after
- stores
- kinetic, gravitational potential, chemical, elastic, nuclear, electrostatic, internal
Core applies this to simple flow diagrams; Supplement to multi-stage examples and Sankey diagrams.
1.7.2Work
Mechanical work done
W = Fd = ΔE
RearrangedF = W / d · d = W / F
- W
- work doneJ
- F
- forceN
- d
- distance moved in the direction of the forcem
- ΔE
- energy transferredJ
1.7.3Energy resources
Efficiency, by energy
efficiency = useful energy output / total energy input
- energy
- both terms in the same unitJ
Multiply by 100% for a percentage. Core needs the idea of efficiency qualitatively; the equation is Supplement.
Efficiency, by power
efficiency = useful power output / total power input
- power
- both terms in the same unitW
Multiply by 100% for a percentage.
1.7.4Power
Power from work done
P = W / t
RearrangedW = Pt · t = W / P
- P
- powerW, kW, MW
- W
- work doneJ
- t
- time takens
Power from energy transferred
P = ΔE / t
- P
- powerW
- ΔE
- energy transferredJ
- t
- time takens
1.8Pressure
Pressure
p = F / A
RearrangedF = pA · A = F / p
- p
- pressureN/m², Pa
- F
- force normal to the surfaceN
- A
- aream², cm²
Change in pressure beneath a liquid surface
Δp = ρgΔh
- Δp
- change in pressurePa
- ρ
- density of the liquidkg/m³
- g
- gravitational field strengthN/kg
- Δh
- change in depthm
Thermal physics
PDF2.1.3Gases and the absolute scale of temperature
Kelvin and Celsius
T (in K) = θ (in °C) + 273
Rearrangedθ (in °C) = T (in K) − 273
- T
- absolute temperatureK
- θ
- temperature°C
−273 °C is absolute zero, where particles have least kinetic energy.
Pressure and volume of a fixed mass of gas
pV = constant
Rearrangedp₁V₁ = p₂V₂
- p
- pressurePa
- V
- volumem³
For a fixed mass of gas at constant temperature. You may also be asked to represent this graphically.
2.2.2Specific heat capacity
Specific heat capacity
c = ΔE / (mΔθ)
RearrangedΔE = mcΔθ · Δθ = ΔE / (mc)
- c
- specific heat capacityJ/(kg °C), J/(g °C)
- ΔE
- energy suppliedJ
- m
- masskg, g
- Δθ
- temperature rise°C
2.2.3Melting, boiling and evaporation
No equations. 0625 does not examine specific latent heat — melting, boiling and evaporation are described in terms of energy and particles.
2.3Transfer of thermal energy
No equations. Conduction, convection and radiation are examined qualitatively and through experiment.
Waves
PDF3.1General properties of waves
Wave speed
v = fλ
Rearrangedf = v / λ · λ = v / f
- v
- wave speedm/s
- f
- frequencyHz, kHz
- λ
- wavelengthm, cm
3.2.1Reflection of light
Law of reflection
angle of incidence = angle of reflection
- i
- angle of incidence, from the normaldegree (°)
- r
- angle of reflection, from the normaldegree (°)
3.2.2Refraction of light
Refractive index from angles
n = sin i / sin r
Rearrangedsin r = sin i / n
- n
- refractive index
- i
- angle of incidencedegree (°)
- r
- angle of refractiondegree (°)
Refractive index from the critical angle
n = 1 / sin c
Rearrangedsin c = 1 / n
- n
- refractive index
- c
- critical angledegree (°)
Refractive index as a ratio of speeds
n = speed in region 1 / speed in region 2
- n
- refractive index
The syllabus defines refractive index as the ratio of the speeds of a wave in two different regions.
3.2.3Thin lenses
No equations. 0625 examines lenses through ray diagrams and image characteristics — the lens equation is not required.
3.3Electromagnetic spectrum
Speed of electromagnetic waves
c = 3.0 × 10⁸ m/s
- c
- speed in a vacuumm/s
Approximately the same in air. All electromagnetic waves travel at this speed in a vacuum, which Core candidates must know qualitatively.
3.4Sound
Speed of sound by an echo
v = 2d / t
- v
- speed of soundm/s
- d
- distance to the reflecting surfacem
- t
- time for the echo to returns
Not printed in the syllabus: it is v = s/t with the pulse counted there and back. The syllabus asks for a method involving a measurement of distance and time.
Depth or distance from an ultrasound pulse
d = vt / 2
- d
- depth or distancem
- v
- wave speed in the mediumm/s
- t
- time for the pulse to returns
Not printed in the syllabus: it is v = s/t with the pulse counted there and back. The syllabus requires depth or distance to be calculated from time and wave speed for sonar, medical scanning and non-destructive testing.
Electricity and magnetism
PDF4.1Simple phenomena of magnetism
No equations. Magnetism at 0625 is field patterns, induced magnetism and the properties of magnetic materials.
4.2.2Electric current
Electric current
I = Q / t
RearrangedQ = It · t = Q / I
- I
- currentA, mA
- Q
- chargeC
- t
- times
Conventional current is from positive to negative; free electrons flow from negative to positive.
4.2.3Electromotive force and potential difference
Electromotive force
E = W / Q
- E
- e.m.f.V
- W
- electrical work done by the sourceJ
- Q
- charge moved around the complete circuitC
Potential difference
V = W / Q
RearrangedW = QV
- V
- potential differenceV, mV, kV
- W
- work done by the charge in the componentJ
- Q
- charge passing throughC
4.2.4Resistance
Resistance
R = V / I
RearrangedV = IR · I = V / R
- R
- resistanceΩ
- V
- potential differenceV
- I
- currentA
Resistance of a metallic conductor
R ∝ l · R ∝ 1 / A
- l
- length of the wirem
- A
- cross-sectional aream²
A proportionality, not a formula: 0625 does not use resistivity. Core candidates state the relationship qualitatively.
4.2.5Electrical energy and electrical power
Electrical power
P = IV
RearrangedI = P / V · V = P / I
- P
- powerW, kW
- I
- currentA
- V
- potential differenceV
Electrical energy
E = IVt
- E
- energy transferredJ, kWh
- I
- currentA
- V
- potential differenceV
- t
- times
The syllabus also expects the kilowatt-hour to be defined and used to calculate the cost of running an appliance.
4.3.2Series and parallel circuits
Resistors in series
R = R₁ + R₂ + …
- R
- combined resistanceΩ
Cells in series
combined e.m.f. = E₁ + E₂ + …
- E
- e.m.f. of each sourceV
Current in a series circuit
current is the same at every point
- I
- currentA
Resistors in parallel
1 / R = 1 / R₁ + 1 / R₂
- R
- combined resistanceΩ
Two resistors. The combined resistance is always less than either resistor alone — which Core candidates state without calculating.
Currents at a junction
sum of currents in = sum of currents out
- I
- current in each branchA
Potential differences in a series circuit
total p.d. = V₁ + V₂ + …
- V
- p.d. across each componentV
Across parallel branches the p.d. is the same as across any one branch.
4.3.3Action and use of circuit components
Two resistors as a potential divider
R₁ / R₂ = V₁ / V₂
- R₁, R₂
- the two resistancesΩ
- V₁, V₂
- the p.d. across eachV
4.4Electrical safety
No new equations. Fuse ratings and trip settings are chosen using P = IV from 4.2.5.
4.5.6The transformer
Transformer turns and voltage
Vp / Vs = Np / Ns
- Vp, Vs
- primary and secondary p.d.V
- Np, Ns
- turns on primary and secondary coils
Transformer at 100% efficiency
IpVp = IsVs
- Ip, Is
- primary and secondary currentA
- Vp, Vs
- primary and secondary p.d.V
Power loss in transmission cables
P = I²R
- P
- power dissipated in the cableW
- I
- currentA
- R
- resistance of the cableΩ
Used to explain why losses are smaller when transmission voltage is greater.
Nuclear physics
PDF5.1.2The nucleus
Nuclide notation
ᴬZX
- A
- nucleon number (mass number)
- Z
- proton number (atomic number)
- X
- chemical symbol of the element
Number of neutrons
number of neutrons = A − Z
- A
- nucleon number
- Z
- proton number
5.2.1Detection of radioactivity
Corrected count rate
corrected count rate = measured count rate − background count rate
- count rate
- counts per second or per minutecounts/s, counts/min
5.2.3Radioactive decay
Alpha decay
A decreases by 4 · Z decreases by 2
- α
- an alpha particle is a helium nucleus, ⁴₂He
Written as a decay equation in nuclide notation.
Beta decay
A unchanged · Z increases by 1
- β
- a beta particle is an electron, ⁰₋₁e
In the nucleus: neutron → proton + electron. β⁺ is not included; β means β⁻.
Gamma emission
A unchanged · Z unchanged
- γ
- electromagnetic radiation from the nucleus
5.2.4Half-life
Half-life
half-life = time for half the nuclei of an isotope to decay
- t½
- half-lifes, min, h, days, weeks, years
Calculations at Core will not include background radiation; Supplement calculates half-life from decay curves that still contain it.
Fraction remaining after n half-lives
fraction remaining = (½)ⁿ
- n
- number of half-lives elapsed
Not printed in the syllabus: it is the definition of half-life applied repeatedly, and it is how most half-life questions are answered.
Space physics
PDF6.1.1The Earth
Average orbital speed
v = 2πr / T
- v
- average orbital speedm/s
- r
- average radius of the orbitm
- T
- orbital periods
6.1.2The Solar System
Travel time of light
t = d / c
- t
- time takens
- d
- distancem
- c
- speed of lightm/s
Not printed in the syllabus: it is v = s/t. The syllabus asks you to calculate the time light takes to cross Solar System distances.
6.2.2Stars
Light-year
1 light-year = 9.5 × 10¹⁵ m
- ly
- distance light travels in one year in a vacuumm
Core candidates define the light-year without being given the value.
6.2.3The Universe
Hubble constant
H₀ = v / d
Rearrangedv = H₀d · d = v / H₀
- H₀
- Hubble constants⁻¹
- v
- speed the galaxy is receding atm/s
- d
- distance of the galaxy from Earthm
Estimated age of the Universe
d / v = 1 / H₀
- 1 / H₀
- an estimate of the age of the Universes
Evidence for all the matter in the Universe having once been at a single point.
Maths you must recall
From the syllabus’s Mathematical requirements rather than its subject content, and just as examinable.
Circumference of a circle
C = 2πr = πd
- C
- circumferencem, cm
- r
- radiusm, cm
- d
- diameterm, cm
Area of a rectangle
A = l × w
- A
- aream², cm²
- l, w
- length and widthm, cm
Area of a triangle
A = ½ × b × h
- A
- aream², cm²
- b
- basem, cm
- h
- perpendicular heightm, cm
This is what the area under a speed–time graph usually comes down to.
Area of a circle
A = πr²
- A
- aream², cm²
- r
- radiusm, cm
Volume of a rectangular block
V = l × w × h
- V
- volumem³, cm³
- l, w, h
- length, width and heightm, cm
Volume of a cylinder
V = πr²h
- V
- volumem³, cm³
- r
- radiusm, cm
- h
- heightm, cm
Pythagoras' theorem
c² = a² + b²
- c
- hypotenuse of a right-angled triangle
- a, b
- the other two sides
How a resultant of two perpendicular vectors is calculated. The sine, cosine and tangent functions are Extended candidates only.
Values to know
Numbers the syllabus expects you to bring with you rather than be given.
- 1.2Acceleration of free fall near the Earth's surface, gEquivalent to a gravitational field strength of 9.8 N/kg.≈ 9.8 m/s²Core
- 2.1.2Absolute zero−273 °C = 0 KCore
- 3.3Speed of electromagnetic waves in a vacuum, cApproximately the same in air.3.0 × 10⁸ m/sSupp.
- 3.4Speed of sound in air≈ 330–350 m/sCore
- 3.4Range of human hearingUltrasound is sound above 20 kHz.20 Hz to 20 000 HzCore
- 5.1.2Relative charges of proton, neutron, electron+1 · 0 · −1Core
- 6.2.2One light-year9.5 × 10¹⁵ mSupp.
- 6.2.3Diameter of the Milky Way≈ 100 000 light-yearsCore
- 6.2.3Current estimate of the Hubble constant, H₀2.2 × 10⁻¹⁸ s⁻¹Supp.