A-Level Chemistry Formula Sheet — Every Equation You Need (AQA 7405)

This is the complete calculation toolkit for AQA A-Level Chemistry (7405), covering both AS and A2. Every formula and equation you need is organised by topic, with a short note on when to use each one — keep it open while you revise, and use it alongside our free A-Level practice tests to check you can actually apply each equation under exam conditions.

Amount of Substance

Formula / EquationWhat it is / When to use it
n = m / MrMoles = mass (g) ÷ molar mass. The starting point for almost every calculation.
PV = nRT, with R = 8.31 J K−1 mol−1Ideal gas equation: P in Pa, V in m3, T in K. Use it to find moles, volume or Mr of a gas.
Number of particles = n × 6.02 × 1023Convert moles into atoms, molecules or ions using the Avogadro constant.
Concentration (mol dm−3) = moles ÷ volume (dm3)For solutions; remember cm3 ÷ 1000 = dm3. Rearrange to moles = concentration × volume for titrations.
Percentage yield = (actual amount ÷ theoretical amount) × 100Use moles or masses, as long as both amounts are in the same units.
Atom economy = (Mr of desired product ÷ sum of Mr of all reactants) × 100Measures how much of the reactants ends up in the useful product; addition reactions score 100%.
Empirical formula: divide each mass or % by Ar, then divide every result by the smallest; molecular formula = (Mr ÷ empirical mass) × empirical formulaThe standard two-step method for finding a formula from composition data and a measured Mr.
Percentage uncertainty = (uncertainty ÷ reading) × 100For apparatus errors; if a reading is taken twice (e.g. start and end of a burette), add the two percentage uncertainties together.

Energetics & Entropy

Formula / EquationWhat it is / When to use it
q = mcΔTHeat change in calorimetry: m = mass of water/solution (g), c = 4.18 J g−1 K−1, ΔT = temperature change.
ΔH = q ÷ nEnthalpy change per mole from a calorimetry experiment; the sign is negative if the temperature rose (exothermic).
Hess cycle (formation route): ΔH = ΣΔfH(products) − ΣΔfH(reactants)Use when you are given enthalpies of formation; go elements → reactants and elements → products.
Hess cycle (combustion route): ΔH = ΣΔcH(reactants) − ΣΔcH(products)Use with enthalpies of combustion; note this one is reactants minus products, the reverse of the formation route.
ΔH = (bonds broken) − (bonds formed)Mean bond enthalpy route: breaking bonds takes energy in (+), forming bonds releases energy (−).
Born–Haber cycle: work around the cycle so ΔfH = atomisation enthalpies + ionisation energies + electron affinities + lattice enthalpyAny one step (usually lattice enthalpy) can be found from all the others; watch the signs and multiply steps for ions formed per formula unit.
ΔS = ΣS(products) − ΣS(reactants)Entropy change of the reaction from standard entropy values; result is in J K−1 mol−1.
ΔG = ΔH − TΔSGibbs free energy: a reaction is feasible when ΔG ≤ 0. Convert ΔS to kJ K−1 mol−1 and T to kelvin first.
T at the feasibility limit = ΔH ÷ ΔSSet ΔG = 0 and rearrange; gives the temperature at which a reaction just becomes (or stops being) feasible.


Kinetics

Formula / EquationWhat it is / When to use it
Rate = k[A]m[B]nRate equation: m and n are the orders with respect to each reactant, found only from experimental data.
Units of k: rearrange k = rate ÷ ([A]m[B]n) and cancelZero order: mol dm−3 s−1; first order: s−1; second order: mol−1 dm3 s−1.
First-order reactions have a constant half-lifeIf successive half-lives are equal, the reaction is first order in that reactant — a quick way to read orders off a graph.
k = A e(−Ea/RT)Arrhenius equation: k rises sharply with temperature because more collisions exceed the activation energy.
ln k = ln A − Ea/RTStraight-line form of the Arrhenius equation, used to plot ln k against 1/T.
Gradient of ln k vs 1/T graph = −Ea/RSo Ea = −gradient × R; remember temperatures must be in kelvin.
Rate-determining step (RDS)The slowest step in a mechanism; only species involved in steps up to and including the RDS appear in the rate equation.

Equilibrium: Kc and Kp

Formula / EquationWhat it is / When to use it
Kc = [products]coefficients ÷ [reactants]coefficientsEquilibrium constant in concentration terms; find its units by substituting mol dm−3 into the expression and cancelling.
Mole fraction xi = ni ÷ ntotalFraction of the total moles of gas mixture made up by gas i; all mole fractions add up to 1.
Partial pressure pi = xi × PtotalEach gas contributes a share of the total pressure in proportion to its mole fraction.
Kp = (partial pressures of products)coefficients ÷ (partial pressures of reactants)coefficientsSame pattern as Kc but for gas mixtures; find units by cancelling the pressure units (kPa or atm).
Temperature changes the value of KRaising the temperature shifts equilibrium in the endothermic direction, so K increases for endothermic reactions and decreases for exothermic ones.
Pressure and catalysts do not change the value of Kp (or Kc)Pressure can shift the position of equilibrium, and a catalyst speeds up both directions equally, but neither alters K itself.

Acids, Bases & Buffers

Formula / EquationWhat it is / When to use it
Kw = [H+][OH−] = 1.00 × 10−14 mol2 dm−6 at 298 KIonic product of water; use it to find [H+] from [OH−] and to calculate the pH of strong bases.
pH = −log10[H+]And the reverse: [H+] = 10−pH.
Strong acid: [H+] = acid concentrationMonoprotic strong acids dissociate completely, so the hydrogen ion concentration equals the acid concentration.
Ka = [H+][A−] ÷ [HA]Acid dissociation constant for a weak acid; the larger Ka, the stronger the weak acid.
Weak acid: [H+] ≈ √(Ka × [HA])Quick weak-acid pH calculation, assuming [H+] = [A−] and that very little HA dissociates.
pKa = −log10 KaConverts very small Ka values into a handy scale; smaller pKa means a stronger acid.
Buffer pH = pKa + log([salt] ÷ [acid])Henderson–Hasselbalch equation for an acidic buffer; [salt] stands for the conjugate base (A−) provided by the salt.
Ksp: for AxBy(s) ⇌ xAy+(aq) + yBx−(aq), Ksp = [Ay+]x[Bx−]ySolubility product of a sparingly soluble salt at saturation; solids never appear in the expression.
Precipitation rule: compare the ionic product with KspIonic product > Ksp: a precipitate forms. Ionic product < Ksp: no precipitate, everything stays dissolved.

Electrochemistry

Formula / EquationWhat it is / When to use it
E°cell = E°(cathode, reduction) − E°(anode, oxidation)Take the more positive electrode potential minus the more negative one; the result is the maximum voltage the cell can deliver.
Feasibility rule: E°cell > 0A positive cell potential means the reaction is thermodynamically feasible (though it may still be slow).
ΔG = −nFE, with F = 96,500 C mol−1Links cell potential to free energy: n = moles of electrons transferred, E = E°cell. A negative ΔG matches a positive Ecell.
Conventional cell representation: oxidation written on the left, e.g. Zn(s) | Zn2+(aq) || Cu2+(aq) | Cu(s)Single lines separate phases, || is the salt bridge, and the highest oxidation states sit nearest the salt bridge.

Spectroscopy & Analysis

Formula / EquationWhat it is / When to use it
A = εcl (Beer–Lambert law)Colorimetry: absorbance A is proportional to concentration c and path length l, so a calibration curve converts absorbance into concentration.
Rf = distance moved by spot ÷ distance moved by solvent frontFrom thin-layer or paper chromatography; compare Rf values with known compounds run under identical conditions.
TMS (tetramethylsilane) is the NMR reference, δ = 0 ppmChemical shifts in 1H and 13C NMR are measured relative to TMS, which is inert, volatile and gives one sharp peak.
Number of peaks in a 13C NMR spectrum = number of different carbon environmentsEquivalent carbons (in identical surroundings) give a single peak, so peak count reveals the symmetry of the molecule.

Periodicity & Atomic Structure

Formula / EquationWhat it is / When to use it
First ionisation energy generally increases across a periodNuclear charge rises while electrons enter the same shell, so shielding is similar and the outer electrons are held more tightly.
Drop at aluminium (Group 3)The outer electron in Al is in a higher-energy 3p sub-shell, further from the nucleus than the 3s electron in Mg, so it is easier to remove.
Drop at sulfur (Group 6)In S the removed electron is paired up in a 3p orbital; repulsion between the paired electrons makes it easier to remove than the single 3p electrons in P.
Relative atomic mass = Σ(m/z × % abundance) ÷ 100Weighted mean mass from a mass spectrum; relative intensities can replace % abundances if they are used consistently.
m/z = mass ÷ chargeMass spectrometry axis; for singly charged ions it equals the ion mass, and the molecular ion peak gives the Mr of the compound.

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