The van 't Hoff equation is a powerful tool in predicting how a reaction's equilibrium constant (K) changes with temperature. It interrelates the equilibrium constant, temperature, standard reaction enthalpy, and the universal gas constant. This equation is represented as:\[\ln{K} = -\dfrac{\Delta \mathrm{H}^{\circ}}{R} \times \dfrac{1}{T} + C\]where:
- \( K \) = Equilibrium constant
- \( \Delta \mathrm{H}^{\circ} \) = Standard enthalpy change of the reaction
- \( R \) = Universal gas constant (8.314 J/mol K)
- \( T \) = Temperature in Kelvin
- \( C \) = An integration constant
The equation emerges from the relationship between thermal dynamics and equilibrium processes. It implies that the equilibrium constant is temperature-dependent, with the enthalpy change playing a significant role in determining the direction and extent of these changes. As the temperature rises, the equilibrium constant shifts according to the sign and magnitude of \( \Delta \mathrm{H}^{\circ} \), giving vital insights into the feasibility and spontaneity of reactions.When using the van 't Hoff equation, analyzing shifts in \( K \) for varying temperatures helps identify the effect of heat (endothermic or exothermic) on a chemical system.