Understanding Gibbs Free Energy and Chemical Equilibrium
Expert reviewed •22 November 2024• 5 minute read
Chemical reactions in nature tend to proceed towards a state of equilibrium. Gibbs free energy helps us predict and understand this behavior. Let's explore how these concepts are interconnected.
The Fundamentals of Gibbs Free Energy
Gibbs free energy (G) represents the energy available in a system to perform useful work at constant temperature and pressure. The change in Gibbs free energy (ΔG) is given by:
ΔG=ΔH−TΔS
where:
ΔH is the change in enthalpy
T is temperature in Kelvin
ΔS is the change in entropy
The value of ΔG tells us about reaction spontaneity:
When ΔG < 0: Reaction is spontaneous (forward direction)
When ΔG > 0: Reaction is non-spontaneous (reverse direction is spontaneous)
When ΔG = 0: System is at equilibrium
Standard Gibbs Free Energy
Standard Gibbs free energy change (ΔG°) refers to the change in Gibbs free energy under standard conditions (1 M concentration, 1 bar pressure, 298.15 K). It's calculated using:
ΔG°=ΔH°−TΔS°
The relationship between ΔG and ΔG° is given by:
ΔG=ΔG°+RTlnQ
where:
R is the gas constant (8.314 J mol⁻¹ K⁻¹)
T is temperature in Kelvin
Q is the reaction quotient
Predicting Reaction Direction
The reaction quotient (Q) helps predict reaction direction: