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IGCSE Physics, Cambridge 0625, Malaysia

The Complete IGCSE Physics 0625 Equations List

Written by IGCSEPhysics Specialist Team · Checked against the Cambridge IGCSE Physics (0625) syllabus · Updated
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Cambridge gives 0625 candidates no formula sheet, and roughly 40% of theory-paper marks involve a calculation. So this list is the single highest-value page you can memorise: every examinable equation, by topic, in words and symbols with units. Equations marked (S) are Supplement, needed for Extended (Papers 2 and 4) only. Everything unmarked is Core, needed by everyone.

How should you use this list?

Do not read it; test against it. Cover the symbols column, write each equation from its word form, then write the units from memory. Two 20-minute sessions a week brings recall under three seconds per equation within a month, which is the speed exam pressure demands.

A note on g: use g=9.8 N/kgg = 9.8\ \text{N/kg} as standard for 0625, but some papers state 10 N/kg10\ \text{N/kg}, so read the question.

Topic 1: Motion, Forces and Energy

The biggest topic and the biggest equation load. These appear in almost every paper.

Equation in wordsSymbolsUnits
average speed = distance ÷ timev=stv = \dfrac{s}{t}m/s, m, s
acceleration = change in velocity ÷ time takena=ΔvΔta = \dfrac{\Delta v}{\Delta t}m/s², m/s, s
density = mass ÷ volumeρ=mV\rho = \dfrac{m}{V}kg/m³, kg, m³
weight = mass × gravitational field strengthW=mgW = mgN, kg, N/kg
gravitational field strength = weight ÷ massg=Wmg = \dfrac{W}{m}N/kg
resultant force = mass × accelerationF=maF = maN, kg, m/s²
spring constant = force ÷ extensionk=Fxk = \dfrac{F}{x}N/m, N, m
moment = force × perpendicular distance from pivotmoment=Fd\text{moment} = FdN m, N, m
momentum = mass × velocity (S)p=mvp = mvkg m/s
impulse = force × time = change in momentum (S)FΔt=Δ(mv)F\Delta t = \Delta(mv)N s = kg m/s
resultant force = change in momentum ÷ time (S)F=ΔpΔtF = \dfrac{\Delta p}{\Delta t}N
kinetic energy = ½ × mass × speed² (S)Ek=12mv2E_k = \dfrac{1}{2}mv^2J, kg, m/s
change in gravitational potential energy = mass × g × change in height (S)ΔEp=mgΔh\Delta E_p = mg\Delta hJ, kg, N/kg, m
work done = force × distance movedW=Fd=ΔEW = Fd = \Delta EJ, N, m
power = work done ÷ time = energy ÷ timeP=Wt=ΔEtP = \dfrac{W}{t} = \dfrac{\Delta E}{t}W, J, s
efficiency = (useful energy output ÷ total energy input) × 100%no symbol%
efficiency = (useful power output ÷ total power input) × 100%no symbol%
pressure = force ÷ areap=FAp = \dfrac{F}{A}Pa, N, m²
change in pressure in a liquid = density × g × change in depth (S)Δp=ρgΔh\Delta p = \rho g \Delta hPa, kg/m³, N/kg, m

Watch the W trap: WW means weight in W=mgW = mg but work in W=FdW = Fd. Context and units tell you which.

Topic 2: Thermal Physics

A short list, but every equation here is Supplement, so Core candidates answer thermal questions qualitatively.

Equation in wordsSymbolsUnits
specific heat capacity = energy ÷ (mass × temperature change) (S)c=ΔEmΔθc = \dfrac{\Delta E}{m\Delta\theta}J/(kg °C), J, kg, °C
pressure × volume = constant, for fixed mass of gas at constant temperature (S)p1V1=p2V2p_1V_1 = p_2V_2Pa, m³ (or kPa, cm³ consistently)
specific latent heat = energy ÷ mass (S)L=ΔEmL = \dfrac{\Delta E}{m}J/kg, J, kg

For the gas law, any pressure and volume units work as long as both sides match. For latent heat, no temperature term appears because the change of state happens at constant temperature, a favourite explain mark.

Topic 3: Waves

Equation in wordsSymbolsUnits
wave speed = frequency × wavelengthv=fλv = f\lambdam/s, Hz, m
refractive index = sin(angle of incidence) ÷ sin(angle of refraction) (S)n=sinisinrn = \dfrac{\sin i}{\sin r}no unit
refractive index = 1 ÷ sin(critical angle) (S)n=1sincn = \dfrac{1}{\sin c}no unit
linear magnification = image height ÷ object height (S)M=hihoM = \dfrac{h_i}{h_o}no unit

Useful values to memorise: light travels at 3×108 m/s3 \times 10^8\ \text{m/s} in a vacuum, and sound travels at roughly 330-350 m/s in air. Echo questions use distance there-and-back, so the path is 2d2d.

Topic 4: Electricity and Magnetism

The densest calculation territory on Paper 4, because equations chain together inside circuit questions.

Equation in wordsSymbolsUnits
charge = current × timeQ=ItQ = ItC, A, s
resistance = potential difference ÷ currentR=VIR = \dfrac{V}{I}Ω, V, A
e.m.f. = work done (by source) ÷ charge (S)E=WQE = \dfrac{W}{Q}V, J, C
potential difference = work done ÷ charge (S)V=WQV = \dfrac{W}{Q}V, J, C
electrical power = current × potential differenceP=IVP = IVW, A, V
electrical power = current² × resistance (S)P=I2RP = I^2RW, A, Ω
electrical energy = current × potential difference × timeE=IVtE = IVtJ, A, V, s
combined resistance in series = sum of resistancesR=R1+R2R = R_1 + R_2Ω
combined resistance in parallel (S)1R=1R1+1R2\dfrac{1}{R} = \dfrac{1}{R_1} + \dfrac{1}{R_2}Ω
resistance is proportional to length and inversely proportional to cross-sectional area (S)RlR \propto l, R1AR \propto \dfrac{1}{A}no unit
transformer voltage ratio = turns ratioVpVs=NpNs\dfrac{V_p}{V_s} = \dfrac{N_p}{N_s}V, turns
ideal transformer: input power = output power (S)IpVp=IsVsI_p V_p = I_s V_sA, V

Two reminders examiners exploit. Parallel resistance: after adding the reciprocals, flip the answer; forgetting the final flip is the most common Paper 4 circuit error. Cable power loss: use P=I2RP = I^2R (it follows from combining P=IVP = IV with V=IRV = IR) and it is why transmission uses high voltage and low current.

Topic 5: Nuclear Physics

Nuclear physics carries almost no equations, but two quantitative tools earn marks.

Tool in wordsSymbolsNotes
nuclide notation: mass number A, proton number Z, element XZAX{}^{A}_{Z}\text{X}A = protons + neutrons; Z = protons
after each half-life, activity (or undecayed nuclei) halvesAA2A4A8A \to \dfrac{A}{2} \to \dfrac{A}{4} \to \dfrac{A}{8}half-life in s, min, h, years

For half-life calculations, build a halving table rather than using formulas. Extended questions add background radiation: subtract the background count before halving (S).

Topic 6: Space Physics

Equation in wordsSymbolsUnits
orbital speed = (2π × orbital radius) ÷ orbital periodv=2πrTv = \dfrac{2\pi r}{T}m/s, m, s
Hubble constant = recession speed ÷ distance (S)H0=vdH_0 = \dfrac{v}{d}s⁻¹, m/s, m
age of the Universe estimate = distance ÷ speed (S)t=dv=1H0t = \dfrac{d}{v} = \dfrac{1}{H_0}s

Cambridge quotes the Hubble constant as 2.2×1018 s12.2 \times 10^{-18}\ \text{s}^{-1}; the question supplies it, but recognising the rearrangement 1H0\dfrac{1}{H_0} as the age estimate is on you.

What is the fastest way to memorise all of these?

Cold self-testing beats re-reading by a wide margin. Write the quantity name, produce the equation and units from memory, mark yourself, and recycle failures into tomorrow’s list. Most students secure the full Core list in two weeks and the Supplement additions in two more.

Three drills that work:

  1. Blank-sheet Fridays: reproduce one topic’s full table from memory weekly.
  2. Reverse drill: given the unit, name every equation that produces it. J has six.
  3. Triangle ban: practise algebraic rearrangement instead of formula triangles, because Supplement equations like Ek=12mv2E_k = \dfrac{1}{2}mv^2 break the triangle method anyway.

A common worry: “There are too many to hold by exam day.” There are about 35, and you already hold more song lyrics than that. Spaced self-testing, ten equations a session, makes the list automatic in under a month. Our tutors open most 1-to-1 classes with a three-minute equation cold test for exactly this reason; it is the cheapest grade insurance in the subject, and it is built into how we run weekly 1.5-hour lessons.

Memorising the list is step one; deploying it is step two. Pair this page with our calculation-method guide, which covers the substitute-rearrange-units routine examiners reward, and test yourself from the word column until the symbols write themselves.

Frequently Asked Questions

Do you get a formula sheet in IGCSE Physics 0625?
No. Cambridge provides no formula sheet for 0625, so every equation must be memorised in symbols, with units. This is the biggest difference from many other boards and the first thing to fix in revision.
How many equations do I need to memorise for IGCSE Physics?
Core candidates need roughly 20 equations. Extended candidates need around 35, because the Supplement adds momentum, energy, latent heat, gas law, refractive index and transformer power equations on top of the Core list.
Which equations are Extended only?
The main Supplement-only equations are momentum and impulse, kinetic and gravitational potential energy, liquid pressure, specific heat capacity, latent heat, the gas law pV = constant, refractive index, magnification, e.m.f. and p.d. as energy per charge, parallel resistance, the ideal-transformer power equation and Hubble's law.
What value of g should I use in 0625?
Use g = 9.8 N/kg, the 0625 standard. Some questions tell you to take g as 10 N/kg, so always read the question stem first and use the value it gives.

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