Gibbs Energy Change

Two competing tendencies drive every chemical and physical change: systems try to shed energy (favouring low HH) and try to spread energy and matter into more ways of arranging themselves (favouring high SS). Tracking spontaneity through the second law alone means computing the entropy change of the surroundings every single time — inconvenient, since most problems only hand you data about the system. J. Willard Gibbs solved this by folding enthalpy and entropy into one new state function, Gibbs energy GG, whose sign at constant temperature and pressure tells you directly whether a process will happen on its own. This article builds G=H−TSG = H - TS from the second law, turns it into the working formula ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S, reads off the spontaneity rules, and links ΔG∘\Delta G^\circ to the equilibrium constant KK.

The core insight

Gibbs energy G=H−TSG = H - TS combines a system's enthalpy and entropy into one state function, so that ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S alone — no data about the surroundings needed — decides spontaneity at constant temperature and pressure.

The core idea

Why a new function is needed. The second law says a process is spontaneous only if ΔStotal=ΔSsystem+ΔSsurroundings≥0\Delta S_{total} = \Delta S_{system} + \Delta S_{surroundings} \geq 0. That is exact, but ΔSsurroundings\Delta S_{surroundings} is awkward to measure directly for a chemical system. Gibbs energy repackages the same physics using only system properties.

The definition. For any system at constant TT:

G=H−TSG = H - TS

where: GG is Gibbs (free) energy, HH is enthalpy, TT is absolute temperature (kelvin), and SS is entropy — all properties of the system alone.

The working equation. At constant temperature and pressure, the change in GG between two states is:

ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S

where: ΔH\Delta H is the enthalpy change (kJ mol⁻¹), ΔS\Delta S is the entropy change (usually given in J K⁻¹ mol⁻¹, so it must be converted to kJ before use), and TT is the constant absolute temperature at which the process occurs.

The spontaneity criterion. This single quantity replaces the need to track the surroundings:

  • ΔG<0\Delta G < 0: the process is spontaneous (exergonic).
  • ΔG>0\Delta G > 0: the process is non-spontaneous in the forward direction — the reverse process is spontaneous instead (endergonic).
  • ΔG=0\Delta G = 0: the system is at equilibrium; forward and reverse rates balance and there is no net driving force either way.

How ΔH\Delta H and ΔS\Delta S interact. Because ΔG\Delta G is a sum of one term independent of TT and one term proportional to TT, the four sign combinations behave very differently:

ΔH\Delta HΔS\Delta SΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta SSpontaneity
−-++always negativespontaneous at all TT
++−-always positivenon-spontaneous at all TT
−-−-depends on TTspontaneous at low TT only
++++depends on TTspontaneous at high TT only

For the two temperature-dependent rows, there is a crossover temperature where the reaction switches character. Setting ΔG=0\Delta G = 0 gives ΔH=TΔS\Delta H = T\Delta S, so:

Tcrossover=ΔHΔST_{crossover} = \frac{\Delta H}{\Delta S}
Figure
A number line showing Gibbs energy change running from negative through zero to positive with spontaneous non spontaneous and equilibrium regions marked
The sign of ΔG decides spontaneity ΔG less than 0 spontaneous ΔG equals 0 equilibrium ΔG greater than 0 non-spontaneous forward reverse process is spontaneous when ΔG greater than 0

Gibbs energy and the equilibrium constant. At standard conditions, ΔG∘\Delta G^\circ links directly to the equilibrium constant KK:

ΔG∘=−RTln⁡K\Delta G^\circ = -RT\ln K

where: R=8.314 J K−1mol−1R = 8.314\ \text{J K}^{-1}\text{mol}^{-1} is the gas constant, TT is absolute temperature, and KK is the equilibrium constant. A large negative ΔG∘\Delta G^\circ gives a large KK (products favoured at equilibrium); a large positive ΔG∘\Delta G^\circ gives a small KK (reactants favoured). This is only an introductory, qualitative-to-basic-quantitative link — full treatment of KK and the reaction quotient QQ belongs to the Equilibrium chapter.

Derivation ADeriving ΔG = ΔH − TΔS as the spontaneity criterion

The goal is to show, starting only from the second law of thermodynamics stated for total entropy and the definitions of enthalpy and Gibbs energy already known from this unit, that a single system-only quantity ΔG\Delta G can replace ΔStotal\Delta S_{total} as the test for spontaneity at constant temperature and pressure, and that its sign gives exactly the spontaneous, non-spontaneous and equilibrium categories used throughout this topic.

Step 1. Start from the second law: a process is spontaneous if and only if ΔStotal=ΔSsystem+ΔSsurroundings≥0\Delta S_{total} = \Delta S_{system} + \Delta S_{surroundings} \geq 0. At constant pressure, the heat released by the system to the surroundings is −ΔHsystem-\Delta H_{system}, and if the surroundings are large enough to stay at constant temperature TT, they absorb this heat reversibly, so ΔSsurroundings=−ΔHsystem/T\Delta S_{surroundings} = -\Delta H_{system}/T.

Step 2. Substitute this into the second law: ΔStotal=ΔSsystem−ΔHsystemT≥0\Delta S_{total} = \Delta S_{system} - \dfrac{\Delta H_{system}}{T} \geq 0. Multiply through by −T-T (a positive quantity, so the inequality flips): −TΔStotal=ΔHsystem−TΔSsystem≤0-T\Delta S_{total} = \Delta H_{system} - T\Delta S_{system} \leq 0.

Step 3. Define ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S (dropping the "system" subscript, since only system quantities remain). From Step 2, ΔG=−TΔStotal\Delta G = -T\Delta S_{total}. Since TT is always positive, the sign of ΔG\Delta G is exactly opposite to the sign of ΔStotal\Delta S_{total}.

Step 4. Read off the criterion. Spontaneous processes need ΔStotal>0\Delta S_{total} > 0, which by Step 3 means ΔG<0\Delta G < 0. Non-spontaneous (forward) processes have ΔStotal<0\Delta S_{total} < 0, meaning ΔG>0\Delta G > 0. Equilibrium, where there is no net driving force in either direction, has ΔStotal=0\Delta S_{total} = 0, meaning ΔG=0\Delta G = 0. This recovers exactly the three-way rule stated above, built entirely from the second law and constant-pressure heat exchange — no new physics was assumed, only a repackaging into a system-only quantity.

Worked example

Problem: For a reaction at 298 K, ΔH=−35.5 kJ mol−1\Delta H = -35.5\ \text{kJ mol}^{-1} and ΔS=−83.6 J K−1mol−1\Delta S = -83.6\ \text{J K}^{-1}\text{mol}^{-1}. Calculate ΔG\Delta G at 298 K, comment on spontaneity, and find the temperature at which the reaction switches from spontaneous to non-spontaneous.

Step 1. Match units before combining. ΔH\Delta H is in kJ mol⁻¹ but ΔS\Delta S is in J K⁻¹mol⁻¹, so convert: ΔS=−83.6 J K−1mol−1=−0.0836 kJ K−1mol−1\Delta S = -83.6\ \text{J K}^{-1}\text{mol}^{-1} = -0.0836\ \text{kJ K}^{-1}\text{mol}^{-1}.

Step 2. Apply ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S at T=298 KT = 298\ \text{K}:

ΔG=−35.5−(298)(−0.0836)=−35.5+24.9=−10.6 kJ mol−1\Delta G = -35.5 - (298)(-0.0836) = -35.5 + 24.9 = -10.6\ \text{kJ mol}^{-1}

Since ΔG<0\Delta G < 0, the reaction is spontaneous at 298 K.

Step 3. Check whether spontaneity depends on TT. Both ΔH\Delta H and ΔS\Delta S are negative here, so from the sign table this reaction is spontaneous only at sufficiently low temperature. Find the crossover temperature by setting ΔG=0\Delta G = 0, i.e., ΔH=TΔS\Delta H = T\Delta S:

Tcrossover=ΔHΔS=−35.5 kJ mol−1−0.0836 kJ K−1mol−1=424.6 KT_{crossover} = \frac{\Delta H}{\Delta S} = \frac{-35.5\ \text{kJ mol}^{-1}}{-0.0836\ \text{kJ K}^{-1}\text{mol}^{-1}} = 424.6\ \text{K}

The reaction stays spontaneous for T<424.6 KT < 424.6\ \text{K} and becomes non-spontaneous above it — consistent with 298 K (well below 424.6 K) giving a negative ΔG\Delta G.

Competitive stretch

Problem: A reaction has equilibrium constant K=1.8×10−5K = 1.8\times10^{-5} at 298 K. Find ΔG∘\Delta G^\circ and state whether the reaction favours reactants or products at equilibrium.

Step 1. Compute ln⁡K\ln K: since K=1.8×10−5K = 1.8\times10^{-5}, ln⁡K=ln⁡(1.8)+ln⁡(10−5)=0.588−11.513=−10.925\ln K = \ln(1.8) + \ln(10^{-5}) = 0.588 - 11.513 = -10.925.

Step 2. Apply ΔG∘=−RTln⁡K\Delta G^\circ = -RT\ln K with R=8.314 J K−1mol−1R = 8.314\ \text{J K}^{-1}\text{mol}^{-1}, T=298 KT = 298\ \text{K}:

ΔG∘=−(8.314)(298)(−10.925)=27 058 J mol−1≈27.1 kJ mol−1\Delta G^\circ = -(8.314)(298)(-10.925) = 27\,058\ \text{J mol}^{-1} \approx 27.1\ \text{kJ mol}^{-1}

Since ΔG∘\Delta G^\circ is positive and K≪1K \ll 1, the reaction strongly favours reactants at equilibrium — the forward reaction is non-spontaneous under standard conditions, exactly as the small KK suggests.

Common traps

  • Unit mismatch: ΔH\Delta H is usually in kJ mol⁻¹ while ΔS\Delta S is in J K⁻¹mol⁻¹ — forgetting to convert before combining them in ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S is the single most common numerical error.
  • Reading ΔG<0\Delta G < 0 as "the reaction will happen fast." Gibbs energy tests thermodynamic feasibility only — reaction rate is a separate (kinetics) question.
  • Applying the sign table by checking only one of ΔH\Delta H or ΔS\Delta S — both signs are needed to know whether spontaneity is universal, never, or temperature-dependent.
  • Treating ΔG∘=−RTln⁡K\Delta G^\circ = -RT\ln K as the full equilibrium story at this level — here it is only an introductory link; KK and reaction quotient QQ are developed properly in the Equilibrium chapter.

Ask the tutor: want to work through more ΔG\Delta G-versus-temperature problems or see how ΔG∘=−RTln⁡K\Delta G^\circ = -RT\ln K connects to the equilibrium constant in more detail?

Why do we need Gibbs energy at all when the second law already tells us spontaneity via total entropy?

The second law is correct but inconvenient: ΔStotal\Delta S_{total} needs the entropy change of the surroundings, which usually is not given directly. Gibbs energy repackages that same second-law inequality (as shown in the derivation above) into ΔG=−TΔStotal\Delta G = -T\Delta S_{total}, a quantity built purely from system properties — ΔH\Delta H, TT, and ΔSsystem\Delta S_{system} — all of which are typically supplied in a problem. It gives the identical spontaneity verdict with far less bookkeeping.

If ΔG is negative, does that mean the reaction happens instantly?

No. ΔG<0\Delta G < 0 only says a reaction is thermodynamically favourable — it will proceed spontaneously given enough time, releasing usable energy as it does. It says nothing about how fast that happens. A reaction can have a strongly negative ΔG\Delta G and still be immeasurably slow at room temperature because of a large activation energy barrier — rate is governed by kinetics, a separate topic from thermodynamics.

How is the crossover temperature T equals ΔH over ΔS actually used in practice?

It marks the single temperature at which ΔG\Delta G switches sign, found by setting ΔG=0\Delta G = 0 in ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S. It is only meaningful when ΔH\Delta H and ΔS\Delta S have the same sign (both negative or both positive), because only then does spontaneity actually depend on TT. In the worked example, Tcrossover=424.6 KT_{crossover} = 424.6\ \text{K} tells us the reaction stops being spontaneous once heated past that point — useful for predicting how a process behaves across a temperature range rather than at one fixed value.

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Where this leads