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17.8 : Calculating Standard Free Energy Changes

The free energy change for a reaction that occurs under the standard conditions of 1 bar pressure and at 298 K is called the standard free energy change. Since free energy is a state function, its value depends only on the conditions of the initial and final states of the system. A convenient and common approach to the calculation of free energy changes for physical and chemical reactions is by use of widely available compilations of standard state thermodynamic data. One method involves the use of standard enthalpies and entropies to compute standard free energy changes, ΔG°, according to the following relation.

HTML static equilibrium equations diagram with ΣFx=0, MA=0, physics concepts, analysis.

The standard free energy change for a reaction may also be calculated from the standard free energy of formation ΔGf° values of the reactants and products involved in the reaction. The standard free energy of formation is the free energy change that accompanies the formation of one mole of a substance from its elements in their standard states. Similar to the standard enthalpy of formation, ΔGf° is by definition zero for elemental substances under standard state conditions. For the reaction

Chromatography method diagram, showing a liquid chromatography column setup for compound separation.

the standard free energy change at room temperature may be calculated as

Static equilibrium concept, ΣFx=0, ΣFy=0, diagram of forces at play, educational physics tool.

The use of free energies of formation to compute free energy changes for reactions as described above is possible because ΔG is a state function, and the approach is analogous to the use of Hess’ Law in computing enthalpy changes. Consider the vaporization of water as an example:

Chemical equilibrium equation Kp=Kc(RT)^Δn, formula in a dynamic equilibrium diagram.

An equation representing this process may be derived by adding the formation reactions for the two phases of water (necessarily reversing the reaction for the liquid phase). The free energy change for the sum reaction is the sum of free energy changes for the two added reactions:

static equilibrium equation ΣFx=0, ΣFy=0, ΣM=0 diagram; forces analysis method

This approach may also be used in cases where a nonspontaneous reaction is enabled by coupling it to a spontaneous reaction. For example, the production of elemental zinc from zinc sulfide is thermodynamically unfavorable, as indicated by a positive value for ΔG°1:

Four-bar linkage mechanism diagram illustrating static equilibrium principles with force vectors.

The industrial process for the production of zinc from sulfidic ores involves coupling this decomposition reaction to the thermodynamically favorable oxidation of sulfur:

Chirality diagram showing enantiomers of a chiral molecule with three-dimensional bond structure.

The coupled reaction exhibits a negative free energy change and is spontaneous:

Chromatography process diagram showing mobile and stationary phases for compound separation.

This process is typically carried out at elevated temperatures, so this result obtained using standard free energy values is just an estimate. The gist of the calculation, however, holds true.

This text is adapted from Openstax, Chemistry 2e, Chapter 16.4: Free Energy.

Tagi

Standard Free Energy ChangeChemical ReactionStandard ConditionStandard GFormationCalcium CarbonateCalcium OxideCarbon DioxideStandard Enthalpy ChangeStandard Entropy ChangeReference TablesStandard Molar Entropies298 KJDifferenceProductsReactantsStoichiometric CoefficientsHydrogen GasChlorine GasHydrogen Chloride Gas

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17.8 : Calculating Standard Free Energy Changes

Thermodynamics

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