Gibbs Energy and Equilibrium
The Gibbs free energy (G) is an essential thermodynamic function that combines enthalpy (H) and entropy (S) to determine the spontaneity of thermodynamic processes at constant temperature and pressure. The Gibbs energy change (
ΔG) for a reaction can be expressed mathematically as:
ΔG = ΔH - TΔS
This equation indicates that the spontaneity of a process depends not only on the change in enthalpy (ΔH) but also on the change in entropy (ΔS) multiplied by the absolute temperature (T).
When ΔG is less than zero (ΔG < 0), the process is spontaneous; when ΔG is greater than zero (ΔG > 0), it is non-spontaneous. At equilibrium, ΔG equals zero (ΔG = 0), indicating no net change in the system. Furthermore, there exists a direct relationship between ΔG and the equilibrium constant (K), summarized by the equation:
ΔG° = -RT ln K
where R is the universal gas constant and T is the temperature in Kelvin. This relationship allows chemists to calculate either Gibbs energy changes from known equilibrium constant values or vice versa. Therefore, understanding Gibbs energy is crucial for predicting the feasibility of reactions and the extent of product formation at equilibrium.