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Free Energy, Nonstandard States, and Equilibrium in Chemical Reactions

Study Guide - Smart Notes

Tailored notes based on your materials, expanded with key definitions, examples, and context.

Free Energy Changes for Nonstandard States

From Standard Free Energy (ΔG°) to Actual Free Energy (ΔG)

In real chemical systems, conditions often differ from the standard state (1 M concentration, 1 atm pressure). The Gibbs free energy change under these nonstandard conditions is given by:

  • Key Equation:

  • R: Universal gas constant, 8.314 J/(mol·K)

  • T: Temperature in Kelvin

  • Q: Reaction quotient, reflecting current concentrations/pressures

Physical Interpretation:

  • When Q = 1 (standard conditions):

  • When Q < K: (forward reaction is spontaneous)

  • When Q > K: (reverse reaction is spontaneous)

  • When Q = K: (system at equilibrium)

The term corrects the standard free energy for the actual conditions of the system.

Free energy vs pressure for water vaporization, showing ΔG negative for evaporation, zero at equilibrium, and positive for condensation

Free Energy and Equilibrium: Relating ΔG° to K

Derivation and Interpretation of ΔG° = −RT ln K

At equilibrium, the reaction quotient Q equals the equilibrium constant K, and the free energy change ΔG is zero. Substituting these values into the key equation yields:

  • Therefore,

  • Or, rearranged:

Implications:

  • Small changes in ΔG° cause large changes in K due to the logarithmic relationship.

  • ΔG° < 0: K > 1 (products favored at equilibrium)

  • ΔG° > 0: K < 1 (reactants favored at equilibrium)

  • ΔG° = 0: K = 1 (reactants and products equally favored)

Free energy curves for K < 1 and K > 1, showing spontaneous direction of reactionFree energy curve for K = 1, showing equilibrium at standard conditions

Summary Table: Relationship Between ΔG° and K

The following table summarizes how the sign and magnitude of ΔG° relate to the equilibrium constant K and the position of equilibrium:

ΔG°rxn

K value

Equilibrium Position

Reaction at Standard Conditions

ΔG° << 0 (large negative)

K >> 1

Products strongly favored

Spontaneous forward

ΔG° < 0 (moderately negative)

K > 1

Products favored

Spontaneous forward

ΔG° = 0

K = 1

Reactants = products

At equilibrium

ΔG° > 0 (moderately positive)

K < 1

Reactants favored

Spontaneous reverse

ΔG° >> 0 (large positive)

K << 1

Reactants strongly favored

Spontaneous reverse

Additional info: Small changes in ΔG° produce large changes in K due to the exponential relationship.

Example: Calculating K from ΔG°rxn

Consider the reaction: N2O4(g) ⇌ 2 NO2(g). Given the following standard free energies of formation:

Table of ΔGf° values for N2O4 and NO2

Calculate ΔG°rxn:

Calculation of ΔG°rxn for the reaction

Calculate K at 298 K:

Calculation of K from ΔG°rxn

Result: K = 0.32, indicating that products are slightly disfavored at standard conditions.

Coupling Reactions: Driving Nonspontaneous Processes

Thermodynamic Coupling in Chemistry and Biology

Some reactions with ΔG > 0 (nonspontaneous) can be made to occur by coupling them with a spontaneous reaction (ΔG < 0) so that the overall ΔG is negative. This principle is fundamental in both industrial and biological processes.

  • Industrial Example: Extraction of iron from iron ore (Fe2O3) is nonspontaneous, but becomes spontaneous when coupled with the combustion of carbon.

  • Biological Example: ATP hydrolysis (ΔG ≈ −30.5 kJ/mol) is coupled to many cellular reactions to make them spontaneous overall.

Diagram showing coupling of ATP hydrolysis with a nonspontaneous reaction

Key Equations in Thermodynamics and Equilibrium

  • Boltzmann Equation (Entropy):

  • Entropy Change (Reversible Process):

  • Entropy of Surroundings:

  • Gibbs Free Energy:

  • Standard Entropy Change:

  • Standard Free Energy Change:

  • Free Energy at Nonstandard Conditions:

  • Relationship to Equilibrium Constant:

Comprehensive Review: Final Takeaways

  1. ΔG = ΔG° + RT ln Q: Corrects standard free energy for actual conditions.

  2. ΔG° = −RT ln K: Master equation linking thermodynamics and equilibrium.

  3. Large negative ΔG° → K ≫ 1 (products favored); large positive ΔG° → K ≪ 1 (reactants favored).

  4. Coupling reactions: Nonspontaneous processes can be driven by coupling with spontaneous ones.

  5. All spontaneous processes are driven by ΔS_universe > 0; ΔG = −TΔS_universe is the practical criterion.

  6. Key equations: S = k ln W; ΔS = q/T; ΔS_surr = −ΔH/T; ΔG = ΔH−TΔS; ΔS°_rxn and ΔG°_rxn formulas; ΔG = ΔG° + RT ln Q; ΔG° = −RT ln K.

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