AP® Chemistry Beta

The equations and constants sheet, explained

On exam day you get a periodic table and a sheet of equations and constants. Here is what each one is for, when to reach for it, and the slips that cost points. The sheet itself is published by the College Board; this page is our own guide to using it.

Three habits that save points

Particles, light and charge

EquationWhat it isWhen you use itLearn it in
F ∝ q₁q₂ / r²Coulomb's law: the attraction between two charges grows with the charges and falls with the square of the distance.Every "why is this ionization energy, radius, lattice energy or boiling point bigger" argument. You rarely calculate with it; you compare both species' charges and distances.Units 1, 2, 3
Periodic Trends
E = hνThe energy of one photon from its frequency.Photoelectron spectroscopy, emission lines, which wavelengths can cause an electronic transition. h = 6.626 × 10⁻³⁴ J·s.Units 1, 3
Properties of Photons
c = λνSpeed of light from wavelength and frequency.Converting a wavelength (often given in nm: change it to m) to a frequency before E = hν. c = 2.998 × 10⁸ m/s.Unit 3
Properties of Photons
N_A = 6.022 × 10²³ mol⁻¹Avogadro's number: particles in one mole.Moving between a count of particles and moles; per-photon energy to per-mole energy.Unit 1
Moles and Molar Mass

Gases, liquids and solutions

EquationWhat it isWhen you use itLearn it in
PV = nRTThe ideal gas law.Moles, molar mass or density of a gas from its pressure, volume and temperature. Temperature in kelvins, and pick the R that matches your units.Unit 3
Ideal Gas Law
P₁V₁/T₁ = P₂V₂/T₂The combined gas law, for a fixed amount of gas.The same gas before and after a change in conditions. Again kelvins only.Unit 3
Ideal Gas Law
P_total = P_A + P_B + …; P_A = X_A × P_totalDalton's law and mole fraction.Gas mixtures, and gas collected over water (subtract the water's vapor pressure).Unit 3
Ideal Gas Law
R = 8.314 J/(mol·K) = 0.08206 L·atm/(mol·K)The gas constant in two sets of units.0.08206 with liters and atmospheres (gas law problems); 8.314 with joules (ΔG° = −RT ln K, the Nernst equation, kinetic energy).Units 3, 9
Ideal Gas Law
STP: 273.15 K and 1.0 atm; 22.4 L/molStandard temperature and pressure, and the molar volume of an ideal gas there.A shortcut only at STP. At any other conditions use PV = nRT.Unit 3
Ideal Gas Law
KE = ½mv²Kinetic energy of a moving particle.Kinetic molecular theory: at the same temperature, lighter particles move faster on average.Unit 3
Kinetic Molecular Theory
M = n_solute / L of solutionMolarity.Every solution calculation: dilution, titration, stoichiometry in solution. Liters of solution, not of solvent.Units 3, 4
Solutions and Mixtures
D = m/V; molar mass = m/nDensity, and molar mass from a mass and an amount.Identifying a gas or liquid; combined with PV = nRT for a gas's molar mass.Units 1, 3
Ideal Gas Law
A = εbcThe Beer-Lambert law: absorbance from molar absorptivity, path length and concentration.Spectrophotometry labs: a calibration line, then a concentration from an absorbance. Also kinetics labs that follow a colored species.Units 3, 5, 7
Beer-Lambert Law

Kinetics

EquationWhat it isWhen you use itLearn it in
ln[A]_t − ln[A]_0 = −ktThe first-order integrated rate law.Concentration after a time, or k from data. If ln[A] against t is a straight line, the reaction is first order (slope −k).Unit 5
Concentration Changes Over Time
1/[A]_t − 1/[A]_0 = ktThe second-order integrated rate law.If 1/[A] against t is a straight line, the reaction is second order (slope k).Unit 5
Concentration Changes Over Time
t½ = 0.693/kThe half-life of a first-order reaction.Only for first order: its half-life does not depend on concentration (radioactive decay, many decompositions).Unit 5
Concentration Changes Over Time

Equilibrium, acids and bases

EquationWhat it isWhen you use itLearn it in
Kc = [C]^c[D]^d / ([A]^a[B]^b); Kp the same with partial pressuresThe equilibrium constant for aA + bB ⇌ cC + dD.Every equilibrium question; Q has the same form with the current values. Leave out pure solids and liquids.Unit 7
Reaction Quotient and Equilibrium Constant
Kw = [H₃O⁺][OH⁻] = 1.0 × 10⁻¹⁴ at 25 °C; pH + pOH = 14.00The ionization of water.Converting between [H₃O⁺] and [OH⁻], or pH and pOH, at 25 °C.Unit 8
Introduction to Acids and Bases
pH = −log[H₃O⁺]; pOH = −log[OH⁻]; pKa = −log KaLogarithmic scales for acidity and acid strength.Base-10 log, never ln. Keep as many decimal places as the concentration has significant figures.Unit 8
Introduction to Acids and Bases
Kw = Ka × Kb; pKa + pKb = pKwThe link between a conjugate acid and base.Getting Ka of NH₄⁺ from Kb of NH₃ (or the reverse) before a buffer or salt calculation.Unit 8
Weak Acid and Base Equilibria
pH = pKa + log([A⁻]/[HA])The Henderson-Hasselbalch equation.Buffer pH from the ratio of conjugate base to weak acid. At half-equivalence the ratio is 1, so pH = pKa. For a basic buffer, use the pKa of the conjugate acid.Unit 8
Henderson-Hasselbalch Equation

Thermodynamics and electrochemistry

EquationWhat it isWhen you use itLearn it in
q = mcΔTHeat absorbed or released when a substance changes temperature.Calorimetry: q of the solution, then ΔH per mole with the opposite sign.Unit 6
Heat Capacity and Calorimetry
ΔH°rxn = Σ ΔH°f(products) − Σ ΔH°f(reactants)Enthalpy of reaction from enthalpies of formation. ΔS° and ΔG° from tables work the same way.Each value times its coefficient; an element in its standard state has ΔH°f = 0 (but not S° = 0).Units 6, 9
Enthalpy of Formation
ΔG° = ΔH° − TΔS°Gibbs free energy from enthalpy and entropy.Whether a process is thermodynamically favored, and at what temperatures. Convert ΔS° from J to kJ first.Unit 9
Gibbs Free Energy and Thermodynamic Favorability
ΔG° = −RT ln KThe link between free energy and the equilibrium constant.K from ΔG° or the reverse. R = 8.314 J/(mol·K), so ΔG° in joules. Natural log here.Unit 9
Free Energy and Equilibrium
ΔG° = −nFE°The link between free energy and cell potential.n is the moles of electrons transferred in the balanced equation. F = 96,485 C/mol e⁻, and 1 V = 1 J/C.Unit 9
Cell Potential and Free Energy
E = E° − (RT/nF) ln QThe Nernst equation: cell potential away from standard conditions.Mostly reasoning: when Q < 1, E > E°; when Q > 1, E < E°; at equilibrium E = 0.Unit 9
Cell Potential Under Nonstandard Conditions
I = q/tCurrent is charge per time (1 A = 1 C/s).Electrolysis: charge from current and time, then moles of electrons with F, then moles of metal from the half-reaction.Unit 9
Electrolysis and Faraday's Law

What is not on the sheet

The exam gives you these values in the question, or expects you to reason without them. None of them is printed on the sheet.

The sheet also lists unit symbols, conversions (1 atm = 760 mm Hg = 760 torr; 1 V = 1 J/C; 1 A = 1 C/s) and the metric prefixes from giga to pico.

Practice with it

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