Skip to main content

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.

1

Motion, forces and energy

PDF

1.1Physical quantities and measurement techniques

  1. 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

  1. Speed

    v = s / t

    Rearrangeds = vtt = s / v

    v
    speedm/s
    s
    distance travelledm
    t
    time takens
  2. Average speed

    average speed = total distance travelled / total time taken

    distance
    the whole journeym
    time
    the whole journeys
  3. Speed from a distance–time graph

    speed = gradient of a distance–time graph

    gradient
    rise ÷ run of a straight-line section
  4. 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.

  5. 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.

  6. Acceleration from a speed–time graph

    acceleration = gradient of a speed–time graph

    gradient
    rise ÷ run

1.3Mass and weight

  1. Gravitational field strength

    g = W / m

    RearrangedW = mgm = 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

  1. Density

    ρ = m / V

    Rearrangedm = ρVV = m / ρ

    ρ
    densityg/cm³, kg/m³
    m
    masskg, g
    V
    volumem³, cm³

1.5.1Effects of forces

  1. Resultant force and acceleration

    F = ma

    Rearrangeda = F / mm = 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.

  2. Spring constant

    k = F / x

    RearrangedF = kxx = 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

  1. Moment of a force

    moment = F × d

    F
    forceN
    d
    perpendicular distance from the pivotm
    moment
    turning effectN m
  2. 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

  1. Momentum

    p = mv

    Rearrangedm = p / vv = p / m

    p
    momentumkg m/s, N s
    m
    masskg
    v
    velocitym/s
  2. Impulse

    impulse = FΔt = Δ(mv)

    F
    forceN
    Δt
    time for which the force actss
    Δ(mv)
    change in momentumkg m/s, N s
  3. Resultant force from momentum

    F = Δp / Δt

    F
    resultant forceN
    Δp
    change in momentumkg m/s
    Δt
    time takens
  4. 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

  1. Kinetic energy

    Ek = ½mv²

    Rearrangedv = √(2Ek / m)

    Ek
    kinetic energyJ
    m
    masskg
    v
    speedm/s
  2. 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
  3. 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

  1. Mechanical work done

    W = Fd = ΔE

    RearrangedF = W / dd = W / F

    W
    work doneJ
    F
    forceN
    d
    distance moved in the direction of the forcem
    ΔE
    energy transferredJ

1.7.3Energy resources

  1. 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.

  2. 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

  1. Power from work done

    P = W / t

    RearrangedW = Ptt = W / P

    P
    powerW, kW, MW
    W
    work doneJ
    t
    time takens
  2. Power from energy transferred

    P = ΔE / t

    P
    powerW
    ΔE
    energy transferredJ
    t
    time takens

1.8Pressure

  1. Pressure

    p = F / A

    RearrangedF = pAA = F / p

    p
    pressureN/m², Pa
    F
    force normal to the surfaceN
    A
    aream², cm²
  2. 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
2

Thermal physics

PDF

2.1.3Gases and the absolute scale of temperature

  1. 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.

  2. Pressure and volume of a fixed mass of gas

    pV = constant

    Rearrangedp₁V₁ = p₂V₂

    p
    pressurePa
    V
    volume

    For a fixed mass of gas at constant temperature. You may also be asked to represent this graphically.

2.2.2Specific heat capacity

  1. Specific heat capacity

    c = ΔE / (mΔθ)

    RearrangedΔE = mcΔθΔθ = 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.

3

Waves

PDF

3.1General properties of waves

  1. Wave speed

    v = fλ

    Rearrangedf = v / λλ = v / f

    v
    wave speedm/s
    f
    frequencyHz, kHz
    λ
    wavelengthm, cm

3.2.1Reflection of light

  1. 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

  1. 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 (°)
  2. Refractive index from the critical angle

    n = 1 / sin c

    Rearrangedsin c = 1 / n

    n
    refractive index
    c
    critical angledegree (°)
  3. 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

  1. 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

  1. 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.

  2. 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.

4

Electricity and magnetism

PDF

4.1Simple phenomena of magnetism

No equations. Magnetism at 0625 is field patterns, induced magnetism and the properties of magnetic materials.

4.2.2Electric current

  1. Electric current

    I = Q / t

    RearrangedQ = Itt = 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

  1. Electromotive force

    E = W / Q

    E
    e.m.f.V
    W
    electrical work done by the sourceJ
    Q
    charge moved around the complete circuitC
  2. 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

  1. Resistance

    R = V / I

    RearrangedV = IRI = V / R

    R
    resistanceΩ
    V
    potential differenceV
    I
    currentA
  2. Resistance of a metallic conductor

    R ∝ l · R ∝ 1 / A

    l
    length of the wirem
    A
    cross-sectional area

    A proportionality, not a formula: 0625 does not use resistivity. Core candidates state the relationship qualitatively.

4.2.5Electrical energy and electrical power

  1. Electrical power

    P = IV

    RearrangedI = P / VV = P / I

    P
    powerW, kW
    I
    currentA
    V
    potential differenceV
  2. 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

  1. Resistors in series

    R = R₁ + R₂ + …

    R
    combined resistanceΩ
  2. Cells in series

    combined e.m.f. = E₁ + E₂ + …

    E
    e.m.f. of each sourceV
  3. Current in a series circuit

    current is the same at every point

    I
    currentA
  4. 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.

  5. Currents at a junction

    sum of currents in = sum of currents out

    I
    current in each branchA
  6. 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

  1. 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

  1. Transformer turns and voltage

    Vp / Vs = Np / Ns

    Vp, Vs
    primary and secondary p.d.V
    Np, Ns
    turns on primary and secondary coils
  2. Transformer at 100% efficiency

    IpVp = IsVs

    Ip, Is
    primary and secondary currentA
    Vp, Vs
    primary and secondary p.d.V
  3. 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.

5

Nuclear physics

PDF

5.1.2The nucleus

  1. Nuclide notation

    ᴬZX

    A
    nucleon number (mass number)
    Z
    proton number (atomic number)
    X
    chemical symbol of the element
  2. Number of neutrons

    number of neutrons = A − Z

    A
    nucleon number
    Z
    proton number

5.2.1Detection of radioactivity

  1. 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

  1. 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.

  2. 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⁻.

  3. Gamma emission

    A unchanged · Z unchanged

    γ
    electromagnetic radiation from the nucleus

5.2.4Half-life

  1. Half-life

    half-life = time for half the nuclei of an isotope to decay

    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.

  2. 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.

6

Space physics

PDF

6.1.1The Earth

  1. 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

  1. 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

  1. 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

  1. Hubble constant

    H₀ = v / d

    Rearrangedv = H₀dd = v / H₀

    H₀
    Hubble constants⁻¹
    v
    speed the galaxy is receding atm/s
    d
    distance of the galaxy from Earthm
  2. 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.

M

Maths you must recall

From the syllabus’s Mathematical requirements rather than its subject content, and just as examinable.

  1. Circumference of a circle

    C = 2πr = πd

    C
    circumferencem, cm
    r
    radiusm, cm
    d
    diameterm, cm
  2. Area of a rectangle

    A = l × w

    A
    aream², cm²
    l, w
    length and widthm, cm
  3. 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.

  4. Area of a circle

    A = πr²

    A
    aream², cm²
    r
    radiusm, cm
  5. Volume of a rectangular block

    V = l × w × h

    V
    volumem³, cm³
    l, w, h
    length, width and heightm, cm
  6. Volume of a cylinder

    V = πr²h

    V
    volumem³, cm³
    r
    radiusm, cm
    h
    heightm, cm
  7. 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.