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University30 min41 / 45

Chemical thermodynamics

Use enthalpy and Hess's law, entropy and Gibbs energy to calculate reaction heats and predict whether a reaction is spontaneous.

Check yourself
In this lesson you will learn
  • Calculate ΔH° from enthalpies of formation and with Hess's law
  • Estimate and calculate the entropy change of a reaction
  • Use ΔG = ΔH − TΔS for spontaneity and ΔG° = −RT ln K for the equilibrium constant

Iron rusts by itself, yet water does not split into hydrogen and oxygen on its own. Most exothermic reactions are spontaneous, but ice melts at room temperature by absorbing heat — an endothermic process can be spontaneous too. So heat alone does not decide. Thermodynamics combines two quantities, enthalpy and entropy, into the Gibbs energy, which tells us exactly whether a reaction is “allowed”.

Enthalpy and Hess's law

The first law of thermodynamics: ΔU = q + w. At constant pressure the expansion work is w = −pΔV, so qp = ΔU + pΔV. This combination is called enthalpy, H = U + pV, so the heat absorbed at constant pressure equals ΔH. ΔH < 0 means exothermic, ΔH > 0 endothermic. H is a state function: its change depends only on the initial and final states, not on the path. This is Hess's law — chemical equations can be added like algebraic ones.

ΔᵣH° = Σ ν · ΔfH°(products) − Σ ν · ΔfH°(reactants)
where:
  • ΔfH°standard enthalpy of formation, kJ/mol; zero for elements in their standard states
  • νstoichiometric coefficient in the equation

A consequence of Hess's law: products minus reactants

SubstanceΔfH°, kJ/molS°, J/(mol·K)
CO₂(g)−393.5213.7
H₂O(l)−285.869.9
CH₄(g)−74.8186.3
NH₃(g)−46.1192.5
CaCO₃(s)−1206.992.9
CaO(s)−635.139.8
N₂(g) / H₂(g) / O₂(g)0191.6 / 130.7 / 205.1
Standard values at 298 K (g gas, l liquid, s solid)
Worked example 1

Calculate the enthalpy of combustion of methane: CH₄(g) + 2O₂(g) → CO₂(g) + 2H₂O(l).

Show solution
ΔH° = [−393.5 + 2 · (−285.8)] − [−74.8 + 2 · 0]
= −965.1 + 74.8 = −890.3 kJ/mol.
That is the heat released by burning 1 mol (16 g) of methane on a gas stove.
Worked example 2 (Hess's law)

C + O₂ → CO₂, ΔH₁ = −393.5 kJ; CO + ½O₂ → CO₂, ΔH₂ = −283.0 kJ. Find the enthalpy of formation of CO (hard to measure directly, because some CO₂ always forms as well).

Show solution
Keep the first equation, reverse the second: CO₂ → CO + ½O₂, ΔH = +283.0 kJ.
Add: C + O₂ + CO₂ → CO₂ + CO + ½O₂ ⇒ C + ½O₂ → CO.
ΔfH°(CO) = −393.5 + 283.0 = −110.5 kJ/mol.
Worked example 3 (bond energies)

Average bond energies: E(H–H) = 436, E(Cl–Cl) = 243, E(H–Cl) = 432 kJ/mol. Estimate ΔH for H₂ + Cl₂ → 2HCl.

Show solution
Broken: 1 H–H + 1 Cl–Cl = 436 + 243 = 679 kJ (energy absorbed).
Formed: 2 H–Cl = 2 · 432 = 864 kJ (energy released).
ΔH ≈ 679 − 864 = −185 kJ — almost exactly the tabulated value (2 · (−92.3) = −184.6 kJ).

Entropy

Entropy measures the number of microstates W of a system: S = k · ln W (Boltzmann's formula). The more disorder, the larger S: solid < liquid < gas. Reactions that increase the number of moles of gas have ΔS > 0. The second law of thermodynamics: in a spontaneous process the entropy of the universe (system + surroundings) increases. The surroundings' entropy change depends on the heat the system gives them: ΔS(surr) = −ΔH / T.

S = k · ln W ΔᵣS° = Σ ν · S°(products) − Σ ν · S°(reactants)
where:
  • kBoltzmann constant, 1.381·10⁻²³ J/K (k = R / Nₐ)
  • Wnumber of microstates consistent with the macrostate
  • S°standard molar entropy, J/(mol·K)

For example, N₂ + 3H₂ → 2NH₃: ΔS° = 2 · 192.5 − (191.6 + 3 · 130.7) = −198.7 J/K (4 mol of gas → 2 mol)

Gibbs energy and spontaneity

Derivation. For a spontaneous process ΔS(universe) = ΔS − ΔH / T > 0. Multiply the inequality by −T (which flips it): ΔH − TΔS < 0. Defining G = H − TS gives ΔG = ΔH − TΔS at constant T and p. So the condition for spontaneity is simply ΔG < 0, expressed entirely through properties of the system.

ΔG = ΔH − T · ΔS ΔG° = −R · T · ln K
where:
  • ΔGchange in Gibbs energy, kJ/mol; ΔG < 0 means spontaneous
  • ΔSentropy change, J/(mol·K)
  • Tabsolute temperature, K
  • R8.314 J/(mol·K)
  • Kequilibrium constant
ΔHΔSResult
−+spontaneous at every temperature
+−never spontaneous
−−at low temperature: T < ΔH / ΔS
++at high temperature: T > ΔH / ΔS
Worked example 4

CaCO₃(s) → CaO(s) + CO₂(g). Using the table, calculate ΔH°, ΔS° and ΔG° at 298 K. Above what temperature does limestone decompose spontaneously?

Show solution
ΔH° = (−635.1 − 393.5) − (−1206.9) = +178.3 kJ.
ΔS° = (39.8 + 213.7) − 92.9 = +160.6 J/K = 0.1606 kJ/K.
ΔG°(298) = 178.3 − 298 · 0.1606 ≈ +130.4 kJ > 0 — no decomposition at room temperature.
Temperature where ΔG = 0: T = ΔH / ΔS = 178 300 / 160.6 ≈ 1110 K (≈ 840 °C). The estimate assumes ΔH and ΔS do not depend on temperature.
Interactive
Loading simulation…
ΔG (kJ, vertical axis) against temperature (K, horizontal axis): ΔG = ΔH − TΔS, with h = ΔH (kJ) and s = ΔS (J/K). The starting values are for CaCO₃ decomposition: the line crosses zero at ≈ 1110 K. Change the signs of h and s to check the four cases in the table.
Worked example 5

For N₂ + 3H₂ ⇌ 2NH₃ at 298 K, ΔG° = −32.8 kJ. Find the equilibrium constant.

Show solution
ln K = −ΔG° / (RT) = 32 800 / (8.314 · 298) ≈ 13.24.
K = exp(13.24) ≈ 5.6·10⁵ — the equilibrium lies far to the right. Yet at 298 K the reaction hardly proceeds: thermodynamics says “allowed”, but kinetics decides how fast.

Key points

  • At constant pressure q = ΔH; ΔᵣH° = Σ ΔfH°(products) − Σ ΔfH°(reactants).
  • Hess's law: ΔH is path-independent; equations can be added, reversed and scaled.
  • S = k ln W; more moles of gas give ΔS > 0; ΔS(surr) = −ΔH / T.
  • ΔG = ΔH − TΔS < 0 means spontaneous; crossover temperature T = ΔH / ΔS.
  • ΔG° = −RT ln K; at 298 K every −5.7 kJ raises K tenfold.

Check yourself

10 questions. Every correct answer earns XP.

1 / 10
For 2H₂(g) + O₂(g) → 2H₂O(l), ΔH = −571.6 kJ. What is ΔH for H₂O(l) → H₂(g) + ½O₂(g)?