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AP Chemistry Notes

9.3.5 Using ΔG° = ΔH° − TΔS° at a Given Temperature

AP Syllabus focus: ‘If ΔH° and ΔS° are known at a temperature, calculate ΔG° directly using ΔG° = ΔH° − TΔS°.’

Gibbs free energy links enthalpy, entropy, and temperature into one criterion for thermodynamic driving force under standard conditions. This page focuses on using ΔG=ΔHTΔS \Delta G^\circ = \Delta H^\circ - T\Delta S^\circ at a specified temperature.

When and why to use ΔG=ΔHTΔS \Delta G^\circ = \Delta H^\circ - T\Delta S^\circ

You use this relationship when you are given (or can determine) standard enthalpy change and standard entropy change for a process and need the standard Gibbs free energy change at a particular temperature.

This approach is especially useful because:

  • Enthalpy captures heat/bond-energy effects.

  • Entropy captures energy dispersal and matter/energy distribution effects.

  • Temperature controls how strongly the entropy term contributes.

A key idea is that the entropy contribution is scaled by temperature, so the same ΔS \Delta S^\circ matters more at higher TT.

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These lines show how ΔG\Delta G varies with temperature for different sign combinations of ΔH\Delta H and ΔS\Delta S. The vertical position relative to ΔG=0\Delta G=0 indicates whether the process is thermodynamically favored, and the temperature where a line crosses zero corresponds to the point where ΔH=TΔS\Delta H = T\Delta S (equilibrium for that process). Source

Key quantities (standard-state context)

Standard Gibbs free energy change, ΔG\Delta G^\circ: The change in Gibbs free energy for a reaction/process when reactants and products are in their standard states; it combines enthalpy and entropy effects at a specified temperature.

Using ΔG \Delta G^\circ is only meaningful when your ΔH \Delta H^\circ and ΔS \Delta S^\circ values refer to the same reaction as written (including physical states) and the same standard-state basis. In typical AP Chemistry usage, standard-state thermodynamic data are tabulated for a stated reference pressure and specified concentrations for solutes; the crucial point here is internal consistency among the values you use.

The equation and what each term means

ΔG=ΔHTΔS \Delta G^\circ = \Delta H^\circ - T\Delta S^\circ

ΔG \Delta G^\circ = standard Gibbs free energy change (energy per mole of reaction as written), typically in kJ mol1 \text{kJ mol}^{-1} or J mol1 \text{J mol}^{-1}

ΔH \Delta H^\circ = standard enthalpy change (energy per mole of reaction as written), typically in kJ mol1 \text{kJ mol}^{-1} or J mol1 \text{J mol}^{-1}

T T = absolute temperature in K \text{K}

ΔS \Delta S^\circ = standard entropy change (energy per mole per kelvin), typically in J mol1K1 \text{J mol}^{-1}\text{K}^{-1}

This equation is a bookkeeping tool: it combines an enthalpy “push” (ΔH\Delta H^\circ) with an entropy “push” (TΔST\Delta S^\circ) to determine the net free-energy change under standard conditions at that temperature.

Unit discipline (the most common source of mistakes)

Because ΔH \Delta H^\circ and TΔS T\Delta S^\circ must be subtracted, they must be in the same energy units.

Practical rules:

  • Always use Kelvin for temperature: T(K)=T(C)+273.15T(\text{K}) = T(^{\circ}\text{C}) + 273.15.

  • If ΔS \Delta S^\circ is given in J mol1K1 \text{J mol}^{-1}\text{K}^{-1} and ΔH \Delta H^\circ is in kJ mol1 \text{kJ mol}^{-1} , convert one so both match.

    • Commonly: convert ΔS \Delta S^\circ to kJ mol1K1 \text{kJ mol}^{-1}\text{K}^{-1} by dividing by 1000.

  • Keep track of the “per mole of reaction” basis:

    • If you scale the balanced equation, ΔH \Delta H^\circ , ΔS \Delta S^\circ , and therefore ΔG \Delta G^\circ all scale by the same factor.

Interpreting the result at the given temperature (without overgeneralising)

After calculating ΔG \Delta G^\circ at the stated temperature:

  • A negative ΔG \Delta G^\circ indicates the reaction/process is thermodynamically favoured under standard conditions at that temperature.

  • A positive ΔG \Delta G^\circ indicates it is not thermodynamically favoured under standard conditions at that temperature.

  • A value near zero suggests little driving force under standard conditions at that temperature.

This interpretation is tied to the specific temperature used in the calculation; changing TT changes the magnitude of the entropy contribution (TΔST\Delta S^\circ), which can shift ΔG \Delta G^\circ even when ΔH \Delta H^\circ and ΔS \Delta S^\circ are treated as constant over the temperature range.

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This table summarizes the four possible sign-combinations of ΔH\Delta H and ΔS\Delta S and the resulting temperature dependence of ΔG\Delta G. It makes the role of the TΔS-T\Delta S term explicit: increasing TT strengthens the entropy contribution and can flip the sign of ΔG\Delta G when ΔH\Delta H and ΔS\Delta S have the same sign. Source

Assumptions and limitations students should state or recognise

Using ΔG=ΔHTΔS \Delta G^\circ = \Delta H^\circ - T\Delta S^\circ cleanly at a “given temperature” rests on assumptions that are usually acceptable in AP-level problems but still worth knowing:

  • ΔH \Delta H^\circ and ΔS \Delta S^\circ are treated as temperature-independent over the range considered (often around 298 K unless stated otherwise).

  • The computed value is standard free energy, not the free energy change for arbitrary (nonstandard) concentrations/pressures.

  • Physical states matter: ΔH \Delta H^\circ , ΔS \Delta S^\circ , and ΔG \Delta G^\circ depend on whether substances are (s), (l), (g), or (aq).

What “at a given temperature” means operationally

To apply the syllabus skill precisely:

  • Use the temperature provided (not automatically 298 K).

  • Convert that temperature to K.

  • Compute the entropy contribution as TΔST\Delta S^\circ with consistent units.

  • Subtract that contribution from ΔH \Delta H^\circ to obtain ΔG \Delta G^\circ for that temperature under standard conditions.

FAQ

Because both $ \Delta H^\circ $ and $ \Delta S^\circ $ can vary with temperature via heat capacities.

For large temperature changes, treating them as constants can noticeably shift $T\Delta S^\circ$ and therefore $ \Delta G^\circ $.

It can be viewed as the temperature-scaled energy dispersal contribution.

In many treatments, it corresponds to the portion of energy change associated with entropy that affects how much energy is available to drive change under standard conditions.

Yes. The equation requires absolute temperature because entropy has units per kelvin.

Using Celsius would shift $T$ by 273.15 and give an incorrect magnitude for $T\Delta S^\circ$ and thus $ \Delta G^\circ $.

A negative $ \Delta S^\circ $ makes $T\Delta S^\circ$ negative, so subtracting it becomes addition: $ \Delta G^\circ = \Delta H^\circ + |T\Delta S^\circ| $.

This means entropy can oppose the process more strongly as temperature rises.

Match the precision of your inputs after unit conversions.

If $T$ is given as an integer kelvin and $ \Delta S^\circ $ has three significant figures, keep intermediate values (like $T\Delta S^\circ$) unrounded, then round $ \Delta G^\circ $ at the end.

Practice Questions

Q1 (3 marks) A reaction has ΔH=+45.0 kJ mol1 \Delta H^\circ = +45.0\ \text{kJ mol}^{-1} and ΔS=+120. J mol1K1 \Delta S^\circ = +120.\ \text{J mol}^{-1}\text{K}^{-1} at 298 K298\ \text{K}. Calculate ΔG \Delta G^\circ at 298 K298\ \text{K}.

  • Converts ΔS \Delta S^\circ to 0.120 kJ mol1K10.120\ \text{kJ mol}^{-1}\text{K}^{-1} (or converts ΔH \Delta H^\circ to J): 1 mark

  • Calculates TΔS=298×0.120=35.8 kJ mol1T\Delta S^\circ = 298 \times 0.120 = 35.8\ \text{kJ mol}^{-1} (or equivalent in J): 1 mark

  • Calculates ΔG=45.035.8=+9.2 kJ mol1 \Delta G^\circ = 45.0 - 35.8 = +9.2\ \text{kJ mol}^{-1} (with correct sign and units): 1 mark

Q2 (6 marks) For a process, ΔH=18.0 kJ mol1 \Delta H^\circ = -18.0\ \text{kJ mol}^{-1} and ΔS=55.0 J mol1K1 \Delta S^\circ = -55.0\ \text{J mol}^{-1}\text{K}^{-1} . (a) Calculate ΔG \Delta G^\circ at 298 K298\ \text{K}. (3 marks)
(b) Calculate ΔG \Delta G^\circ at 350 K350\ \text{K}. (2 marks)
(c) State, based on your values, which temperature gives the more thermodynamically favoured standard free-energy change. (1 mark)

  • Unit conversion for entropy: 0.0550 kJ mol1K1-0.0550\ \text{kJ mol}^{-1}\text{K}^{-1} (or consistent alternative): 1 mark

  • TΔST\Delta S^\circ at 298 K: 298×(0.0550)=16.4 kJ mol1298 \times (-0.0550) = -16.4\ \text{kJ mol}^{-1}: 1 mark

  • ΔG298=18.0(16.4)=1.6 kJ mol1 \Delta G^\circ_{298} = -18.0 - (-16.4) = -1.6\ \text{kJ mol}^{-1}, correct sign/units: 1 mark (b)

  • TΔST\Delta S^\circ at 350 K: 350×(0.0550)=19.3 kJ mol1350 \times (-0.0550) = -19.3\ \text{kJ mol}^{-1}: 1 mark

  • ΔG350=18.0(19.3)=+1.3 kJ mol1 \Delta G^\circ_{350} = -18.0 - (-19.3) = +1.3\ \text{kJ mol}^{-1}, correct sign/units: 1 mark (c)

  • Identifies 298 K298\ \text{K} as more favoured because ΔG \Delta G^\circ is more negative (negative vs positive): 1 mark

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