Calculating Equilibrium Constant from Gibbs Free Energy – Haber Process Examples
Relationship Between Gibbs Free Energy (ΔG°) and the Equilibrium Constant (K)
- Fundamental equation introduced/used in class:
ΔG∘=−RTlnK - Rearranged for solving K:
lnK=−RTΔG∘
K=e−RTΔG∘ - Meaning of symbols
• ΔG∘ = standard Gibbs free-energy change (units: \text{kJ·mol}^{-1}, but must be converted to \text{J·mol}^{-1} when used with R).
• R = ideal-gas constant = 8.314\ \text{J·mol}^{-1}\text{K}^{-1}.
• T = absolute temperature in Kelvin.
• K = equilibrium constant (unitless) representing (reactants)(products) at equilibrium.
Worked Example 1 – Haber Process at 25 °C
- Reaction: N<em>2(g)+3H</em>2(g)⇌2NH3(g)
- Given/previously calculated: \Delta G^{\circ}_{25^{\circ}\text{C}} = -33.3\ \text{kJ·mol}^{-1}.
- Convert ΔG∘ to joules: -33.3\ \text{kJ·mol}^{-1}\times1000 = -3.33\times10^{4}\ \text{J·mol}^{-1}.
- Insert into rearranged formula:
lnK=−(8.314)(298)−3.33×104=13.4 - Exponentiate to isolate K:
K=e13.4≈7×105 - Interpretation:
• A very large K (≫1) indicates the equilibrium position at 25 °C lies heavily toward products (NH₃).
• Numerically, product concentration dominates; reactants are depleted.
Worked Example 2 – Haber Process at 500 °C
- Temperature conversion: 500∘C=500+273=773 K.
- Provided \Delta G^{\circ}_{773\,\text{K}} = +61\ \text{kJ·mol}^{-1} (extracted from earlier slide).
- Convert to joules: +61\ \text{kJ·mol}^{-1}\times1000 = 6.10\times10^{4}\ \text{J·mol}^{-1}.
- Calculate lnK:
lnK=−(8.314)(773)6.10×104=−9.49 - Solve for K:
K=e−9.49≈7.45×10−5 - Interpretation:
• K ≪ 1 implies equilibrium now favors reactants (N₂ and H₂).
• Demonstrates temperature’s dramatic effect on equilibrium position for the Haber reaction.
Theoretical & Practical Significance
- Temperature Dependence:
• As temperature increases from 298 K to 773 K, ΔG∘ shifts from negative to positive, flipping the favored side.
• Consistent with Le Châtelier’s Principle for an exothermic formation of NH₃: raising T drives equilibrium toward reactants. - Industrial Relevance:
• Although low temperatures favor NH₃ yield (large K), practical production balances kinetics (rate) and thermodynamics.
• High pressure and optimized catalysts are employed in real Haber plants to offset the reduced K at elevated T. - Conceptual Link:
• Connects back to prior lectures on spontaneity: \Delta G^{\circ}<0 ↔ spontaneous under standard conditions.
• Shows direct quantitative bridge between thermodynamic driving force (free energy) and observable equilibrium composition.
Calculation Reminders & Common Pitfalls
- Always convert kJ→J when pairing ΔG∘ with R.
- Temperature must be Kelvin.
- Sign discipline: negative signs in ΔG∘ or rearranged formulae can invert interpretation if mishandled.
- Exponentials grow fast; check with orders-of-magnitude reasoning (e.g., lnK=13 → K≈105).
Quick Reference Equations
- Core identity: ΔG=ΔG∘+RTlnQ (specializes to Q=K at equilibrium).
- Equilibrium expression for Haber process (all gases):
K=[N</em>2][H2]3[NH<em>3]2 (activities if not ideal).
Take-Home Messages
- You can translate a measured/calculated ΔG∘ directly into an equilibrium constant at any temperature.
- The sign and magnitude of ΔG∘ dictate how far a reaction proceeds under standard conditions.
- For exothermic industrial syntheses like ammonia formation, optimizing T involves a trade-off between favorable K (low T) and acceptable reaction rates (higher T).