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2027 exam · Reference sheet

AP® Chemistry reference sheet (2027), explained

College Board's official 2027 PDF has two pages: tables of unit symbols, unit conversions and metric prefixes, then equations and constants grouped by topic. College Board's student exam page says you also get a periodic table for the whole exam. This page goes through every equation and constant on the sheet in plain words: what each symbol means, its unit, when to use it, the mistake students make most, and where we teach it.

The official sheet: AP Chemistry Exam Reference Information (PDF, College Board) (opens in a new tab). Keep it open next to this page. We link to it instead of copying it, so you always see College Board's current version.

Checked against the 2027 version on October 5, 2026. The explanations are ours, not College Board's.

Using the sheet on exam day

  • You have the sheet for the whole exam, both sections, in the testing app and as a paper booklet you can do scratch work in. Learn its layout before exam day so you aren't hunting for an equation under time pressure.
  • The sheet never tells you when an equation applies. It lists t1/2=0.693kt_{1/2} = \frac{0.693}{k} without saying it's only for first-order reactions, and Henderson–Hasselbalch without saying it's only for buffers. Knowing the conditions is your job.
  • Watch letters that mean two things. On the sheet, cc is the speed of light, the concentration in A=εbcA = \varepsilon bc, the specific heat in q=mcΔTq = mc\Delta T, and a coefficient in KcK_c. Bold M\boldsymbol{M} is molar mass and plain MM is molarity. qq is charge in Coulomb's law and I=qtI = \frac{q}{t}, but heat in q=mcΔTq = mc\Delta T.
  • Use the metric prefix table to convert before you plug in: 500 nm is 500 × 10⁻⁹ m, and 25 kJ is 25,000 J. Pick the gas constant whose units match your problem: 0.08206 for liters and atm, 8.314 for joules.
  • Some things you need are not on the sheet at all, like Ecell∘=Ecathode∘−Eanode∘E^\circ_{\text{cell}} = E^\circ_{\text{cathode}} - E^\circ_{\text{anode}}, Hess's law and KspK_{sp} setups. See the list at the end of this page.

Constants and conversions

Planck's constant
h=6.626×10−34 J s\displaystyle h = 6.626 \times 10^{-34}\ \text{J s}
Use it in E=hνE = h\nu to turn a photon's frequency into its energy in joules.
Speed of light
c=2.998×108 m s−1\displaystyle c = 2.998 \times 10^{8}\ \text{m s}^{-1}
Use it in c=λνc = \lambda\nu to go between wavelength and frequency. Wavelength has to be in meters to match.
Avogadro's number
6.022×1023 mol−1\displaystyle 6.022 \times 10^{23}\ \text{mol}^{-1}
Use it to go between moles and particles: atoms, molecules, ions or photons. Multiply moles by it to get a count, divide a count by it to get moles.
Gas constant, in joules
R=8.314 J mol−1 K−1\displaystyle R = 8.314\ \text{J mol}^{-1}\ \text{K}^{-1}
Use this value when energy is involved: ΔG∘=−RTln⁡K\Delta G^\circ = -RT\ln K and the Nernst equation. It gives an answer in joules, so convert if the rest of your work is in kJ.
Gas constant, in liters and atmospheres
R=0.08206 L atm mol−1 K−1\displaystyle R = 0.08206\ \text{L atm mol}^{-1}\ \text{K}^{-1}
Use this value in PV=nRTPV = nRT when pressure is in atm and volume is in liters.
Standard temperature and pressure
STP=273.15 K and 1.0 atm\displaystyle \text{STP} = 273.15\ \text{K and } 1.0\ \text{atm}
STP means 0 °C and 1 atm. Don't mix it up with the 25 °C (298 K) used for standard thermodynamic values like ΔH∘\Delta H^\circ.
Molar volume of an ideal gas at STP
Ideal gas at STP=22.4 L mol−1\displaystyle \text{Ideal gas at STP} = 22.4\ \text{L mol}^{-1}
A shortcut for gas stoichiometry: at STP, 1 mol of any ideal gas takes up 22.4 L. Use it only at STP; anywhere else, use PV=nRTPV = nRT.
Faraday's constant
F=96,485 coulombs/1 mol e−\displaystyle F = 96{,}485\ \text{coulombs} / 1\ \text{mol}\ e^-
The charge on one mole of electrons. Use it in ΔG∘=−nFE∘\Delta G^\circ = -nFE^\circ, the Nernst equation, and electrolysis problems that turn coulombs into moles of electrons.
Hertz
1 hertz=1 s−1\displaystyle 1\ \text{hertz} = 1\ \text{s}^{-1}
Frequency ν\nu is in hertz, which is the same as per second. That's why hνh\nu comes out in joules.
Pressure units
1 atm=760 mm Hg=760 torr\displaystyle 1\ \text{atm} = 760\ \text{mm Hg} = 760\ \text{torr}
Convert pressures to atm before using R=0.08206R = 0.08206. For example, 380 mm Hg is 0.500 atm.
Celsius to kelvin
K=∘C+273.15\displaystyle \text{K} = {}^\circ\text{C} + 273.15
Every gas law and every thermodynamics equation with TT in it needs kelvin. A temperature change ΔT\Delta T is the same size in °C and K.
Volt
1 volt=1 joule1 coulomb\displaystyle 1\ \text{volt} = \dfrac{1\ \text{joule}}{1\ \text{coulomb}}
This is why nFE∘nFE^\circ comes out in joules: coulombs times volts is joules.
Ampere
1 ampere=1 coulomb1 second\displaystyle 1\ \text{ampere} = \dfrac{1\ \text{coulomb}}{1\ \text{second}}
Current in amperes times time in seconds gives charge in coulombs, which you need in electrolysis problems.

Atomic structure

Light as photons, and the force between charged particles that explains periodic trends.

Energy of a photon

E=hν\displaystyle E = h\nu

What the symbols mean

EE
energy of one photon
Unit: J
hh
Planck's constant, 6.626 × 10⁻³⁴ J·s
Unit: J·s
ν\nu
frequency of the light (the Greek letter nu, not a v)
Unit: s⁻¹ (Hz)

Use it when: Use it when you know the frequency of light and need the energy of one photon, or the other way around. It also links an electron's energy jump to the light it absorbs or emits.

Watch out: This gives the energy of one photon, not a mole of them. If the problem wants kJ/mol, multiply by Avogadro's number and divide by 1000.

Try it: What is the energy of one photon of light with a wavelength of 500. nm?

Answer: First find the frequency: ν=cλ=2.998×108 m/s500.×10−9 m=5.996×1014 s−1\nu = \frac{c}{\lambda} = \frac{2.998 \times 10^8\ \text{m/s}}{500. \times 10^{-9}\ \text{m}} = 5.996 \times 10^{14}\ \text{s}^{-1}. Then E=hν=(6.626×10−34)(5.996×1014)=3.97×10−19 JE = h\nu = (6.626 \times 10^{-34})(5.996 \times 10^{14}) = 3.97 \times 10^{-19}\ \text{J}.

Learn it: 3.12 Properties of Photons · 1.6 Photoelectron Spectroscopy · 3.11 Spectroscopy and the Electromagnetic Spectrum

Speed of light, wavelength and frequency

c=λν\displaystyle c = \lambda\nu

What the symbols mean

cc
speed of light, 2.998 × 10⁸ m/s
Unit: m/s
λ\lambda
wavelength
Unit: m
ν\nu
frequency
Unit: s⁻¹ (Hz)

Use it when: Use it to switch between wavelength and frequency. Problems often give a wavelength in nm, so you need this before E=hνE = h\nu.

Watch out: Forgetting to convert nanometers to meters. 1 nm = 10⁻⁹ m, so 500 nm is 5.00 × 10⁻⁷ m.

Learn it: 3.11 Spectroscopy and the Electromagnetic Spectrum · 3.12 Properties of Photons

Coulomb's law

Fcoulombic∝q1q2r2\displaystyle F_{\text{coulombic}} \propto \dfrac{q_1 q_2}{r^2}

What the symbols mean

FcoulombicF_{\text{coulombic}}
the force of attraction or repulsion between two charges
Unit: N
q1,q2q_1, q_2
the two charges, like a nucleus and an electron, or two ions
Unit: C
rr
the distance between the charges
Unit: m
∝\propto
is proportional to: the sheet gives no constant, so use it to compare, not to calculate
Unit: none

Use it when: Use it to explain trends: why ionization energy goes up across a period (more protons, same shell), why atoms get bigger down a group, and why MgO has a stronger lattice than NaCl (bigger charges, smaller ions).

Watch out: Saying only one factor changes. In an explanation, name both: the charge (like the number of protons, or the ion charges) and the distance (like the shell number, or the ionic radii), and say which way each pushes the force.

Learn it: 1.5 Atomic Structure and Electron Configuration · 1.7 Periodic Trends · 2.3 Structure of Ionic Solids

Gases, liquids, and solutions

Gas laws, moles and mass, molarity, and measuring concentration with light.

Combined gas law

P1V1T1=P2V2T2\displaystyle \dfrac{P_1V_1}{T_1} = \dfrac{P_2V_2}{T_2}

What the symbols mean

P1,P2P_1, P_2
pressure before and after
Unit: atm, or any unit as long as both match
V1,V2V_1, V_2
volume before and after
Unit: L, or any unit as long as both match
T1,T2T_1, T_2
temperature before and after
Unit: K

Use it when: Use it when the same sample of gas (fixed moles) changes conditions and you need the new pressure, volume or temperature. If one variable stays constant, just leave it out of both sides.

Watch out: Using °C. A gas at 20 °C isn't half as hot as one at 40 °C, so the ratio only works in kelvin. Add 273.15 first.

Learn it: 3.4 Ideal Gas Law

Ideal gas law

PV=nRT\displaystyle PV = nRT

What the symbols mean

PP
pressure
Unit: atm
VV
volume
Unit: L
nn
number of moles of gas
Unit: mol
RR
gas constant, 0.08206 L·atm/(mol·K) with these units
Unit: L·atm/(mol·K)
TT
temperature
Unit: K

Use it when: Use it when a problem gives three of pressure, volume, moles and temperature for one gas sample and asks for the fourth. Pair it with n=mMn = \frac{m}{\boldsymbol{M}} to find a gas's molar mass.

Watch out: Mismatched units. With R=0.08206R = 0.08206, pressure must be in atm, volume in liters and temperature in kelvin. Convert mm Hg, mL and °C before you plug in.

Try it: What is the pressure of 0.500 mol of gas in a 5.00 L container at 27 °C?

Answer: Convert to kelvin: 27 + 273.15 = 300.15 K. Then P=nRTV=(0.500)(0.08206)(300.15)5.00=2.46 atmP = \frac{nRT}{V} = \frac{(0.500)(0.08206)(300.15)}{5.00} = 2.46\ \text{atm}.

Learn it: 3.4 Ideal Gas Law · 3.6 Deviation from Ideal Gas Law

Partial pressure from mole fraction

PA=Ptotal×XA, where XA=moles Atotal moles\displaystyle P_A = P_{\text{total}} \times X_A, \text{ where } X_A = \dfrac{\text{moles A}}{\text{total moles}}

What the symbols mean

PAP_A
partial pressure of gas A, the pressure it would have alone in the container
Unit: atm
PtotalP_{\text{total}}
total pressure of the gas mixture
Unit: atm
XAX_A
mole fraction of A: its share of the total moles, between 0 and 1
Unit: none

Use it when: Use it in a gas mixture when you know the total pressure and the moles of each gas, and need one gas's pressure.

Watch out: Using mass fraction instead of mole fraction. Convert grams of each gas to moles first.

Learn it: 3.4 Ideal Gas Law

Total pressure of a gas mixture

Ptotal=PA+PB+PC+…\displaystyle P_{\text{total}} = P_A + P_B + P_C + \dots

What the symbols mean

PtotalP_{\text{total}}
total pressure of the mixture
Unit: atm
PA,PB,PCP_A, P_B, P_C
partial pressures of each gas in the mixture
Unit: atm

Use it when: Use it when gases share a container and you need the total pressure, or one gas's pressure from the total. A common case is a gas collected over water, where you subtract the water vapor pressure.

Watch out: Forgetting a gas, especially water vapor when a gas is collected over water. Its partial pressure counts toward the total.

Learn it: 3.4 Ideal Gas Law

Moles from mass

n=mM\displaystyle n = \dfrac{m}{\boldsymbol{M}}

What the symbols mean

nn
number of moles
Unit: mol
mm
mass of the sample
Unit: g
M\boldsymbol{M}
molar mass, from the periodic table (bold M on the sheet)
Unit: g/mol

Use it when: Use it every time you go between grams and moles, which is the first step of almost every stoichiometry problem.

Watch out: Mixing up bold M\boldsymbol{M} (molar mass, g/mol) with plain MM (molarity, mol/L). The sheet uses both, so check which one the equation means.

Learn it: 1.1 Moles and Molar Mass · 4.5 Stoichiometry

Density

D=mV\displaystyle D = \dfrac{m}{V}

What the symbols mean

DD
density
Unit: g/L for gases, g/mL for liquids and solids
mm
mass
Unit: g
VV
volume
Unit: L or mL

Use it when: Use it on its own, or with PV=nRTPV = nRT and n=mMn = \frac{m}{\boldsymbol{M}} to find a gas's density or molar mass at a given pressure and temperature.

Watch out: Mixing g/L and g/mL. Gas densities are usually given in g/L, and 1 g/mL = 1000 g/L, so keep track of which volume unit you used.

Learn it: 3.4 Ideal Gas Law

Kinetic energy

KE=12mv2\displaystyle KE = \dfrac{1}{2}mv^2

What the symbols mean

KEKE
kinetic energy of a moving particle
Unit: J
mm
mass of the particle
Unit: kg
vv
velocity (speed) of the particle (a plain v, not the Greek nu)
Unit: m/s

Use it when: Use it with kinetic molecular theory: at the same temperature, all gases have the same average kinetic energy, so lighter molecules must move faster.

Watch out: Thinking heavier molecules have more kinetic energy at the same temperature. Average KE depends only on temperature; a heavier gas just has a lower average speed.

Learn it: 3.5 Kinetic Molecular Theory

Molarity

M=nsoluteLsolution\displaystyle M = \dfrac{n_{\text{solute}}}{\text{L}_{\text{solution}}}

What the symbols mean

MM
molarity, the concentration of a solution
Unit: mol/L (M)
nsoluten_{\text{solute}}
moles of the dissolved substance
Unit: mol
Lsolution\text{L}_{\text{solution}}
volume of the whole solution in liters
Unit: L

Use it when: Use it to find a concentration, or to find moles from a volume and concentration (moles = M × L). Titration and solution stoichiometry problems use it constantly.

Watch out: Using milliliters, or the volume of solvent instead of the total solution. Convert mL to L (divide by 1000) and use the final solution volume.

Learn it: 3.7 Solutions and Mixtures · 4.5 Stoichiometry · 4.6 Introduction to Titration

Beer–Lambert law

A=εbc\displaystyle A = \varepsilon bc

What the symbols mean

AA
absorbance, read from the spectrophotometer
Unit: none
ε\varepsilon
molar absorptivity: how strongly the substance absorbs at that wavelength
Unit: L/(mol·cm), also written M⁻¹ cm⁻¹
bb
path length, the width of the cuvette the light passes through
Unit: cm
cc
concentration (here c is not the speed of light)
Unit: mol/L

Use it when: Use it when a lab measures absorbance to find a concentration. Absorbance is directly proportional to concentration, so a calibration graph of A against c is a straight line.

Watch out: Treating cc as the speed of light. In this equation it's concentration. Also remember ε\varepsilon depends on the wavelength, so measurements must be at the same wavelength.

Learn it: 3.13 Beer-Lambert Law

Kinetics

The integrated rate laws for zero-, first- and second-order reactions, and half-life.

Zero-order integrated rate law

[A]t−[A]0=−kt\displaystyle [\text{A}]_t - [\text{A}]_0 = -kt

What the symbols mean

[A]t[\text{A}]_t
concentration of reactant A at time t
Unit: mol/L
[A]0[\text{A}]_0
starting concentration of A
Unit: mol/L
kk
rate constant
Unit: mol/(L·s), or M/s
tt
time
Unit: s

Use it when: Use it for a zero-order reaction, where the rate doesn't depend on concentration. A graph of [A] against time is a straight line with slope −k-k.

Watch out: Using it without checking the order. Only use it when [A] against time is the straight-line graph.

Learn it: 5.3 Concentration Changes Over Time

First-order integrated rate law

ln⁡[A]t−ln⁡[A]0=−kt\displaystyle \ln[\text{A}]_t - \ln[\text{A}]_0 = -kt

What the symbols mean

ln⁡[A]t\ln[\text{A}]_t
natural log of the concentration of A at time t
Unit: none
ln⁡[A]0\ln[\text{A}]_0
natural log of the starting concentration
Unit: none
kk
rate constant
Unit: s⁻¹
tt
time
Unit: s

Use it when: Use it for a first-order reaction, including radioactive decay. A graph of ln[A] against time is a straight line with slope −k-k.

Watch out: Using log (base 10) instead of ln (natural log). On your calculator, press ln, and undo it with exe^x, not 10x10^x.

Try it: A first-order reaction has k=0.0231 s−1k = 0.0231\ \text{s}^{-1}. If [A]0=0.800 M[\text{A}]_0 = 0.800\ \text{M}, what is [A] after 60.0 s?

Answer: ln⁡[A]t=ln⁡(0.800)−(0.0231)(60.0)=−0.223−1.386=−1.609\ln[\text{A}]_t = \ln(0.800) - (0.0231)(60.0) = -0.223 - 1.386 = -1.609. Then [A]t=e−1.609=0.200 M[\text{A}]_t = e^{-1.609} = 0.200\ \text{M}. That's two half-lives, since t1/2=0.6930.0231=30.0 st_{1/2} = \frac{0.693}{0.0231} = 30.0\ \text{s}.

Learn it: 5.3 Concentration Changes Over Time

Second-order integrated rate law

1[A]t−1[A]0=kt\displaystyle \dfrac{1}{[\text{A}]_t} - \dfrac{1}{[\text{A}]_0} = kt

What the symbols mean

1[A]t\frac{1}{[\text{A}]_t}
one over the concentration of A at time t
Unit: L/mol
1[A]0\frac{1}{[\text{A}]_0}
one over the starting concentration
Unit: L/mol
kk
rate constant
Unit: L/(mol·s), or M⁻¹ s⁻¹
tt
time
Unit: s

Use it when: Use it for a second-order reaction in one reactant. A graph of 1/[A] against time is a straight line with a positive slope equal to kk.

Watch out: Getting the sign wrong. This one is +kt+kt, not −kt-kt, because 1/[A] goes up as [A] goes down.

Learn it: 5.3 Concentration Changes Over Time

Half-life of a first-order reaction

t1/2=0.693k\displaystyle t_{1/2} = \dfrac{0.693}{k}

What the symbols mean

t1/2t_{1/2}
half-life, the time for half the reactant to be used up
Unit: s
kk
first-order rate constant
Unit: s⁻¹
0.6930.693
ln 2, rounded
Unit: none

Use it when: Use it for first-order reactions to go between kk and the half-life. A first-order half-life stays the same no matter how much reactant is left.

Watch out: Using it for zero- or second-order reactions. The sheet doesn't say so, but this equation is only true for first order. For other orders the half-life changes as the concentration drops.

Learn it: 5.3 Concentration Changes Over Time

Equilibrium

Writing equilibrium constants from concentrations or gas pressures. The sheet's list of equilibrium constants names five: KcK_c (molar concentrations), KpK_p (gas pressures), KwK_w (water), KaK_a (acid) and KbK_b (base).

Equilibrium constant in concentrations

Kc=[C]c[D]d[A]a[B]b, where aA+bB⇄cC+dD\displaystyle K_c = \dfrac{[\text{C}]^c[\text{D}]^d}{[\text{A}]^a[\text{B}]^b}, \text{ where } a\text{A} + b\text{B} \rightleftarrows c\text{C} + d\text{D}

What the symbols mean

KcK_c
equilibrium constant written with molar concentrations
Unit: none
[A],[B],[C],[D][\text{A}], [\text{B}], [\text{C}], [\text{D}]
concentrations at equilibrium
Unit: mol/L
a,b,c,da, b, c, d
coefficients from the balanced equation (here c is a coefficient, not concentration)
Unit: none

Use it when: Use it to write the KK expression for any balanced reaction, to calculate KK from equilibrium concentrations, or to find a missing concentration. Put current, non-equilibrium values in the same form and you get QQ.

Watch out: Two classic slips: forgetting the coefficients as exponents, and putting pure solids and liquids in the expression. Leave out anything labeled (s) or (l), like solid CaCO₃ or liquid H₂O.

Try it: For N₂(g) + 3H₂(g) ⇌ 2NH₃(g), the equilibrium concentrations are [N₂] = 0.50 M, [H₂] = 0.20 M and [NH₃] = 0.10 M. Find KcK_c.

Answer: Kc=[NH3]2[N2][H2]3=(0.10)2(0.50)(0.20)3=0.0100.0040=2.5K_c = \frac{[\text{NH}_3]^2}{[\text{N}_2][\text{H}_2]^3} = \frac{(0.10)^2}{(0.50)(0.20)^3} = \frac{0.010}{0.0040} = 2.5. Without the exponents you'd get 1.0, which is wrong.

Learn it: 7.3 Reaction Quotient and Equilibrium Constant · 7.4 Calculating the Equilibrium Constant

Equilibrium constant in partial pressures

Kp=(PC)c(PD)d(PA)a(PB)b\displaystyle K_p = \dfrac{(P_\text{C})^c(P_\text{D})^d}{(P_\text{A})^a(P_\text{B})^b}

What the symbols mean

KpK_p
equilibrium constant written with gas pressures
Unit: none
PA,PB,PC,PDP_\text{A}, P_\text{B}, P_\text{C}, P_\text{D}
partial pressures of each gas at equilibrium
Unit: atm
a,b,c,da, b, c, d
coefficients from the balanced equation
Unit: none

Use it when: Use it for gas-phase equilibria when the problem gives partial pressures instead of concentrations.

Watch out: Including solids, liquids or dissolved species. KpK_p uses only gases, each raised to its coefficient.

Learn it: 7.3 Reaction Quotient and Equilibrium Constant · 7.4 Calculating the Equilibrium Constant

Acids and bases

On the sheet these sit under Equilibrium: water's equilibrium, pH, acid and base constants, and the buffer equation.

Ionization of water

Kw=[H3O+][OH−]=1.0×10−14 at 25∘C\displaystyle K_w = [\text{H}_3\text{O}^+][\text{OH}^-] = 1.0 \times 10^{-14} \text{ at } 25^\circ\text{C}

What the symbols mean

KwK_w
the equilibrium constant for water
Unit: none
[H3O+][\text{H}_3\text{O}^+]
hydronium ion concentration
Unit: mol/L
[OH−][\text{OH}^-]
hydroxide ion concentration
Unit: mol/L

Use it when: Use it to find [OH⁻] from [H₃O⁺] or the other way around, in any water solution at 25 °C.

Watch out: Using 1.0 × 10⁻¹⁴ at other temperatures. KwK_w grows as water warms, so pure water at a higher temperature has a pH below 7 and is still neutral.

Learn it: 8.1 Introduction to Acids and Bases · 8.2 pH and pOH of Strong Acids and Bases

pH plus pOH

pKw=14=pH+pOH at 25∘C\displaystyle \text{p}K_w = 14 = \text{pH} + \text{pOH} \text{ at } 25^\circ\text{C}

What the symbols mean

pKw\text{p}K_w
negative log of KwK_w
Unit: none
pH\text{pH}
negative log of [H₃O⁺]
Unit: none
pOH\text{pOH}
negative log of [OH⁻]
Unit: none

Use it when: Use it to switch between pH and pOH. For a base, it's often easiest to find pOH first, then subtract from 14.

Watch out: Stopping at pOH when the question asks for pH. For bases, check which one you reported.

Learn it: 8.1 Introduction to Acids and Bases · 8.2 pH and pOH of Strong Acids and Bases

pH and pOH

pH=−log⁡[H3O+],pOH=−log⁡[OH−]\displaystyle \text{pH} = -\log[\text{H}_3\text{O}^+], \quad \text{pOH} = -\log[\text{OH}^-]

What the symbols mean

pH\text{pH}
a log scale of acidity: lower means more acidic
Unit: none
pOH\text{pOH}
the same scale for hydroxide
Unit: none
log⁡\log
base-10 log
Unit: none

Use it when: Use it to turn a concentration into pH or pOH. To go back, [H3O+]=10−pH[\text{H}_3\text{O}^+] = 10^{-\text{pH}}, which isn't printed on the sheet. For a strong acid, [H₃O⁺] equals the acid's concentration.

Watch out: Pressing ln instead of log, or dropping the minus sign. A pH should come out between about 0 and 14 for normal solutions; a negative answer for a dilute acid means a sign slip.

Try it: A solution has [OH⁻] = 2.0 × 10⁻⁵ M at 25 °C. What is its pH?

Answer: pOH=−log⁡(2.0×10−5)=4.70\text{pOH} = -\log(2.0 \times 10^{-5}) = 4.70. Then pH=14−4.70=9.30\text{pH} = 14 - 4.70 = 9.30.

Learn it: 8.1 Introduction to Acids and Bases · 8.2 pH and pOH of Strong Acids and Bases

Acid and base ionization constants

Ka=[H3O+][A−][HA],Kb=[OH−][HB+][B]\displaystyle K_a = \dfrac{[\text{H}_3\text{O}^+][\text{A}^-]}{[\text{HA}]}, \quad K_b = \dfrac{[\text{OH}^-][\text{HB}^+]}{[\text{B}]}

What the symbols mean

KaK_a
acid ionization constant: bigger means a stronger acid
Unit: none
KbK_b
base ionization constant: bigger means a stronger base
Unit: none
[HA],[A−][\text{HA}], [\text{A}^-]
concentrations of the weak acid and its conjugate base
Unit: mol/L
[B],[HB+][\text{B}], [\text{HB}^+]
concentrations of the weak base and its conjugate acid
Unit: mol/L

Use it when: Use them to find the pH of a weak acid or weak base solution, usually with an ICE table. For a weak acid alone, [H3O+]=[A−]=x[\text{H}_3\text{O}^+] = [\text{A}^-] = x, so Ka≈x2[HA]0K_a \approx \frac{x^2}{[\text{HA}]_0}.

Watch out: Using them for strong acids or bases, which ionize completely and don't need an equilibrium setup. Also, water is a liquid, so it never appears in these expressions.

Learn it: 8.3 Weak Acid and Base Equilibria

pKa and pKb

pKa=−log⁡Ka,pKb=−log⁡Kb\displaystyle \text{p}K_a = -\log K_a, \quad \text{p}K_b = -\log K_b

What the symbols mean

pKa\text{p}K_a
negative log of KaK_a
Unit: none
pKb\text{p}K_b
negative log of KbK_b
Unit: none

Use it when: Use it to compare acid strengths quickly or to get pKa\text{p}K_a for the Henderson–Hasselbalch equation.

Watch out: Flipping the trend. A smaller pKa\text{p}K_a means a larger KaK_a, so a stronger acid.

Learn it: 8.3 Weak Acid and Base Equilibria · 8.7 pH and pKa

Conjugate acid–base pairs

Kw=Ka×Kb,pKw=pKa+pKb\displaystyle K_w = K_a \times K_b, \quad \text{p}K_w = \text{p}K_a + \text{p}K_b

What the symbols mean

KaK_a
KaK_a of the acid in a conjugate pair
Unit: none
KbK_b
KbK_b of its conjugate base
Unit: none
KwK_w
1.0 × 10⁻¹⁴ at 25 °C
Unit: none

Use it when: Use it when you know KaK_a for an acid like HF and need KbK_b for its conjugate base F⁻, or the other way around.

Watch out: Using it for an acid and a base that aren't a conjugate pair. It only links HA with its own A⁻, or B with its own HB⁺.

Learn it: 8.3 Weak Acid and Base Equilibria

Henderson–Hasselbalch equation

pH=pKa+log⁡[A−][HA]\displaystyle \text{pH} = \text{p}K_a + \log\dfrac{[\text{A}^-]}{[\text{HA}]}

What the symbols mean

pKa\text{p}K_a
pKa\text{p}K_a of the weak acid in the buffer
Unit: none
[A−][\text{A}^-]
concentration (or moles) of the conjugate base
Unit: mol/L
[HA][\text{HA}]
concentration (or moles) of the weak acid
Unit: mol/L

Use it when: Use it for a buffer, a solution with real amounts of both a weak acid and its conjugate base. When they're equal, the log term is zero and pH = pKa.

Watch out: Using it when there's no buffer, like a weak acid alone or a strong acid. It also only works with the ratio base over acid; flipping it gives the wrong sign on the log.

Try it: A buffer has 0.20 M acetate (A⁻) and 0.10 M acetic acid (HA). The pKa\text{p}K_a of acetic acid is 4.74. What is the pH?

Answer: pH=4.74+log⁡0.200.10=4.74+0.30=5.04\text{pH} = 4.74 + \log\frac{0.20}{0.10} = 4.74 + 0.30 = 5.04. More base than acid, so the pH is above the pKa\text{p}K_a.

Learn it: 8.9 Henderson-Hasselbalch Equation · 8.8 Properties of Buffers

Thermodynamics

Heat, enthalpy, entropy and free energy. The sheet chains ΔG∘=ΔH∘−TΔS∘=−RTln⁡K=−nFE∘\Delta G^\circ = \Delta H^\circ - T\Delta S^\circ = -RT\ln K = -nFE^\circ into one block; here each relation gets its own entry, and the last one is under Electrochemistry.

Heat and temperature change

q=mcΔT\displaystyle q = mc\Delta T

What the symbols mean

qq
heat absorbed or released (here q is heat, not charge)
Unit: J
mm
mass of the substance being heated, often the water or solution
Unit: g
cc
specific heat capacity (water is 4.18 J/(g·°C))
Unit: J/(g·°C)
ΔT\Delta T
temperature change, final minus initial
Unit: °C or K (same size)

Use it when: Use it in calorimetry to find the heat gained or lost by water or a solution from its temperature change.

Watch out: Getting the sign of the reaction's heat wrong. If the water warms up, qq for the water is positive, so the reaction released heat and its ΔH\Delta H is negative.

Try it: 50.0 g of water (c = 4.18 J/(g·°C)) warms by 6.00 °C. How much heat did it absorb?

Answer: q=mcΔT=(50.0)(4.18)(6.00)=1.25×103 Jq = mc\Delta T = (50.0)(4.18)(6.00) = 1.25 \times 10^3\ \text{J}, or 1.25 kJ.

Learn it: 6.4 Heat Capacity and Calorimetry · 6.3 Heat Transfer and Thermal Equilibrium

Enthalpy change from enthalpies of formation

ΔHreaction∘=∑ΔHf products∘−∑ΔHf reactants∘\displaystyle \Delta H^\circ_{\text{reaction}} = \sum \Delta H^\circ_{f\ \text{products}} - \sum \Delta H^\circ_{f\ \text{reactants}}

What the symbols mean

ΔHreaction∘\Delta H^\circ_{\text{reaction}}
standard enthalpy change of the reaction: negative means exothermic
Unit: kJ/mol
ΔHf∘\Delta H^\circ_f
standard enthalpy of formation of each substance, from a table
Unit: kJ/mol
∑\sum
add up, after multiplying each by its coefficient
Unit: none

Use it when: Use it when a problem gives a table of ΔHf∘\Delta H^\circ_f values and asks for the reaction's ΔH∘\Delta H^\circ.

Watch out: Forgetting to multiply by coefficients, or flipping the order. It's products minus reactants. Elements in their standard state, like O₂(g), have ΔHf∘=0\Delta H^\circ_f = 0.

Learn it: 6.8 Enthalpy of Formation

Entropy change from standard entropies

ΔSreaction∘=∑Sproducts∘−∑Sreactants∘\displaystyle \Delta S^\circ_{\text{reaction}} = \sum S^\circ_{\text{products}} - \sum S^\circ_{\text{reactants}}

What the symbols mean

ΔSreaction∘\Delta S^\circ_{\text{reaction}}
standard entropy change of the reaction
Unit: J/(mol·K)
S∘S^\circ
standard (absolute) entropy of each substance, from a table
Unit: J/(mol·K)

Use it when: Use it when a problem gives S∘S^\circ values and asks for ΔS∘\Delta S^\circ of a reaction.

Watch out: Setting S∘=0S^\circ = 0 for elements. Unlike ΔHf∘\Delta H^\circ_f, an element's S∘S^\circ is not zero, so include every substance. Also note it's in J, not kJ.

Learn it: 9.2 Absolute Entropy and Entropy Change

Free energy change from free energies of formation

ΔGreaction∘=∑ΔGf products∘−∑ΔGf reactants∘\displaystyle \Delta G^\circ_{\text{reaction}} = \sum \Delta G^\circ_{f\ \text{products}} - \sum \Delta G^\circ_{f\ \text{reactants}}

What the symbols mean

ΔGreaction∘\Delta G^\circ_{\text{reaction}}
standard Gibbs free energy change: negative means thermodynamically favorable
Unit: kJ/mol
ΔGf∘\Delta G^\circ_f
standard free energy of formation of each substance, from a table
Unit: kJ/mol

Use it when: Use it when a table gives ΔGf∘\Delta G^\circ_f values. If it gives ΔH∘\Delta H^\circ and ΔS∘\Delta S^\circ instead, use ΔG∘=ΔH∘−TΔS∘\Delta G^\circ = \Delta H^\circ - T\Delta S^\circ.

Watch out: Forgetting the coefficients, just like with enthalpy. Elements in their standard state have ΔGf∘=0\Delta G^\circ_f = 0.

Learn it: 9.3 Gibbs Free Energy and Thermodynamic Favorability

Free energy from enthalpy and entropy

ΔG∘=ΔH∘−TΔS∘\displaystyle \Delta G^\circ = \Delta H^\circ - T\Delta S^\circ

What the symbols mean

ΔG∘\Delta G^\circ
standard free energy change: negative means thermodynamically favorable
Unit: kJ/mol
ΔH∘\Delta H^\circ
standard enthalpy change
Unit: kJ/mol
TT
temperature
Unit: K
ΔS∘\Delta S^\circ
standard entropy change
Unit: J/(mol·K)

Use it when: Use it to decide if a reaction is favorable at a given temperature, or to find the temperature where it switches (set ΔG∘=0\Delta G^\circ = 0, so T=ΔH∘ΔS∘T = \frac{\Delta H^\circ}{\Delta S^\circ}).

Watch out: Mixing kJ and J. ΔH∘\Delta H^\circ is usually in kJ and ΔS∘\Delta S^\circ in J/K, so divide ΔS∘\Delta S^\circ by 1000 first. And use kelvin, not °C.

Try it: For N₂ + 3H₂ → 2NH₃, ΔH∘=−92.2 kJ/mol\Delta H^\circ = -92.2\ \text{kJ/mol} and ΔS∘=−198.7 J/(mol⋅K)\Delta S^\circ = -198.7\ \text{J/(mol·K)}. Find ΔG∘\Delta G^\circ at 298 K.

Answer: Convert: ΔS∘=−0.1987 kJ/(mol⋅K)\Delta S^\circ = -0.1987\ \text{kJ/(mol·K)}. Then ΔG∘=−92.2−(298)(−0.1987)=−92.2+59.2=−33.0 kJ/mol\Delta G^\circ = -92.2 - (298)(-0.1987) = -92.2 + 59.2 = -33.0\ \text{kJ/mol}, so it's favorable at 298 K.

Learn it: 9.3 Gibbs Free Energy and Thermodynamic Favorability

Free energy and the equilibrium constant

ΔG∘=−RTln⁡K\displaystyle \Delta G^\circ = -RT\ln K

What the symbols mean

ΔG∘\Delta G^\circ
standard free energy change
Unit: J/mol
RR
gas constant, 8.314 J/(mol·K)
Unit: J/(mol·K)
TT
temperature
Unit: K
KK
equilibrium constant
Unit: none

Use it when: Use it to go between ΔG∘\Delta G^\circ and KK. Negative ΔG∘\Delta G^\circ means K>1K > 1 (products favored); positive means K<1K < 1.

Watch out: Two at once: using R=0.08206R = 0.08206 instead of 8.314, and leaving ΔG∘\Delta G^\circ in kJ. With 8.314, ΔG∘\Delta G^\circ must be in J. It's also ln, not log.

Learn it: 9.5 Free Energy and Equilibrium

Electrochemistry

Cell potential, free energy and electrolysis. Faraday's constant is in the constants list above.

Free energy and cell potential

ΔG∘=−nFE∘\displaystyle \Delta G^\circ = -nFE^\circ

What the symbols mean

ΔG∘\Delta G^\circ
standard free energy change
Unit: J/mol
nn
number of moles of electrons transferred in the balanced redox reaction
Unit: mol e⁻
FF
Faraday's constant, 96,485 C/mol e⁻
Unit: C/mol e⁻
E∘E^\circ
standard cell potential
Unit: V

Use it when: Use it to go between a cell's standard potential and ΔG∘\Delta G^\circ. A positive E∘E^\circ gives a negative ΔG∘\Delta G^\circ: a favorable, galvanic cell.

Watch out: Using moles of reactant for nn. It's the moles of electrons transferred, found by balancing the half-reactions. Don't multiply E∘E^\circ by coefficients either; potentials don't scale.

Try it: A zinc–copper cell transfers 2 electrons and has E∘=1.10 VE^\circ = 1.10\ \text{V}. Find ΔG∘\Delta G^\circ.

Answer: ΔG∘=−(2)(96,485)(1.10)=−2.12×105 J/mol\Delta G^\circ = -(2)(96{,}485)(1.10) = -2.12 \times 10^5\ \text{J/mol}, or −212 kJ/mol.

Learn it: 9.9 Cell Potential and Free Energy

Current

I=qt\displaystyle I = \dfrac{q}{t}

What the symbols mean

II
current
Unit: A
qq
charge (here q is charge, not heat)
Unit: C
tt
time
Unit: s

Use it when: Use it in electrolysis: current × time gives coulombs, Faraday's constant turns coulombs into moles of electrons, and the half-reaction turns those into moles of metal.

Watch out: Leaving time in minutes or hours. Convert to seconds first, since 1 A = 1 C/s.

Try it: A current of 2.00 A runs for 965 s through a Cu²⁺ solution. What mass of copper plates out? (Cu²⁺ + 2e⁻ → Cu, molar mass 63.55 g/mol)

Answer: q=It=(2.00)(965)=1930 Cq = It = (2.00)(965) = 1930\ \text{C}, which is 193096,485=0.0200 mol e−\frac{1930}{96{,}485} = 0.0200\ \text{mol}\ e^-. Two electrons per Cu gives 0.0100 mol Cu, and 0.0100×63.55=0.636 g0.0100 \times 63.55 = 0.636\ \text{g}.

Learn it: 9.11 Electrolysis and Faraday's Law

Nernst equation

Ecell=Ecell∘−RTnFln⁡Q\displaystyle E_{\text{cell}} = E^\circ_{\text{cell}} - \dfrac{RT}{nF}\ln Q

What the symbols mean

EcellE_{\text{cell}}
cell potential under the actual conditions
Unit: V
Ecell∘E^\circ_{\text{cell}}
standard cell potential (1 M solutions, 1 atm gases)
Unit: V
RR
gas constant, 8.314 J/(mol·K)
Unit: J/(mol·K)
TT
temperature
Unit: K
nn
moles of electrons transferred
Unit: mol e⁻
FF
Faraday's constant, 96,485 C/mol e⁻
Unit: C/mol e⁻
QQ
reaction quotient for the cell reaction
Unit: none

Use it when: Use it, or just its logic, when concentrations aren't standard. If Q<1Q < 1, ln⁡Q\ln Q is negative and EcellE_{\text{cell}} is bigger than Ecell∘E^\circ_{\text{cell}}; if Q>1Q > 1, it's smaller.

Watch out: Getting the direction backward. Many questions only ask whether the voltage goes up or down, so reason from QQ: more product makes QQ bigger and the voltage lower.

Learn it: 9.10 Cell Potential Under Nonstandard Conditions

Not on the sheet: know these

The exam expects you to know these without being given them.

  • Standard cell potential from half-cells

    Ecell∘=Ecathode∘−Eanode∘\displaystyle E^\circ_{\text{cell}} = E^\circ_{\text{cathode}} - E^\circ_{\text{anode}}

    Problems give a table of standard reduction potentials and expect you to combine them. Use both values as reduction potentials, and never multiply them by coefficients. A positive answer means a galvanic cell.

    Learn it: 9.8 Galvanic (Voltaic) and Electrolytic Cells · 9.9 Cell Potential and Free Energy

  • Enthalpy from bond enthalpies

    ΔH∘=∑(bonds broken)−∑(bonds formed)\displaystyle \Delta H^\circ = \sum \text{(bonds broken)} - \sum \text{(bonds formed)}

    Breaking bonds takes energy and forming them releases it. Note this is reactants minus products, the opposite order from the formation-enthalpy equation on the sheet.

    Learn it: 6.7 Bond Enthalpies

  • Hess's law

    To combine reactions: reverse a reaction and you flip the sign of its ΔH\Delta H; multiply a reaction by a number and you multiply its ΔH\Delta H by the same number. Then add the ΔH\Delta H values.

    Learn it: 6.9 Hess's Law

  • Heat lost equals heat gained

    qsystem=−qsurroundings\displaystyle q_{\text{system}} = -q_{\text{surroundings}}

    In calorimetry, the heat the water gains is the heat the reaction loses. So ΔH\Delta H for the reaction is −qwater-q_{\text{water}} divided by the moles that reacted.

    Learn it: 6.3 Heat Transfer and Thermal Equilibrium · 6.4 Heat Capacity and Calorimetry

  • Q compared with K

    If Q<KQ < K, the reaction shifts forward toward products. If Q>KQ > K, it shifts in reverse. If Q=KQ = K, it's at equilibrium.

    Learn it: 7.3 Reaction Quotient and Equilibrium Constant · 7.10 Reaction Quotient and Le Châtelier's Principle

  • K for reversed or multiplied reactions

    Kreverse=1K,Ktimes n=Kn\displaystyle K_{\text{reverse}} = \dfrac{1}{K}, \quad K_{\text{times } n} = K^n

    Reverse a reaction and its new KK is the reciprocal. Multiply all coefficients by nn and raise KK to the nn. Add two reactions and multiply their KK values.

    Learn it: 7.6 Properties of the Equilibrium Constant

  • Solubility product and molar solubility

    CaF2: Ksp=[Ca2+][F−]2=(s)(2s)2=4s3\displaystyle \text{CaF}_2\text{: } K_{sp} = [\text{Ca}^{2+}][\text{F}^-]^2 = (s)(2s)^2 = 4s^3

    KspK_{sp} follows the same rules as any KK: the solid is left out, and coefficients become exponents. Write each ion's concentration in terms of the molar solubility ss to go between them.

    Learn it: 7.11 Introduction to Solubility Equilibria · 7.12 Common-Ion Effect

  • Dilution

    M1V1=M2V2\displaystyle M_1V_1 = M_2V_2

    Adding water doesn't change the moles of solute, so molarity times volume stays the same. Use it to find a new concentration after diluting.

    Learn it: 3.7 Solutions and Mixtures · 4.6 Introduction to Titration

  • Percent composition and empirical formulas

    mass percent=mass of elementmass of compound×100%\displaystyle \text{mass percent} = \dfrac{\text{mass of element}}{\text{mass of compound}} \times 100\%

    To find an empirical formula, turn each mass percent into grams (assume 100 g), then into moles, then divide by the smallest number of moles to get the whole-number ratio.

    Learn it: 1.3 Elemental Composition of Pure Substances

  • pH equals pKa at half-equivalence

    pH=pKa\displaystyle \text{pH} = \text{p}K_a

    Halfway to the equivalence point in a weak acid titration, half the acid has become its conjugate base, so [HA] = [A⁻]. Read the pH there off the curve and you have the pKa\text{p}K_a.

    Learn it: 8.5 Acid-Base Titrations · 8.9 Henderson-Hasselbalch Equation