

Introduction to Gibbs Free Energy
The Gibbs free energy, also commonly known as the Gibbs function, Gibbs energy, or free enthalpy, is a thermodynamic potential that is used to measure the maximum amount of work done in any given thermodynamic system when the temperature and pressure of the system are kept constant. Gibbs free energy is denoted by the letter G. Its value is usually expressed in either Joules or Kilojoules as it is also a form of energy. Gibbs free energy is defined as the maximum amount of work done that can be extracted from a closed thermodynamic system.
Gibbs energy is a thermodynamic property and it was determined by American scientist Josiah Willard Gibbs in the year 1876 when he was conducting experiments to predict the behaviour of systems when combined together or whether a process could take place simultaneously and spontaneously at a given temperature. Gibbs free energy was also known as available energy. Gibbs free energy can be visualized as the total amount of useful energy present in a thermodynamic system that can be utilized to perform some work.
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Gibbs Energy
Gibbs energy is also known as Gibbs free energy, it is one of the four thermodynamic potentials. Gibbs free energy is equal to the difference in enthalpy of the system with the product of the temperature and entropy. The equation is given as:
G = H - TS
Where,
G = Gibbs free energy
H = enthalpy
T = temperature
S = entropy
Gibbs free energy is a state function thus it doesn’t depend on the path (i.e., its path independent entity). Thus, the change in Gibbs free energy will be equal to the difference in the change in enthalpy with the product of temperature and entropy change of the system.
ΔG = ΔH - Δ(TS)
If the reaction is carried out under constant temperature i.e., assuming that the reaction is isothermal in nature,ΔT=0 then:
ΔG = ΔH - TΔS
This equation is called the Gibbs Helmholtz equation.
Now, depending on the value of the change in Gibbs free energy, we can define many new reactions:
Suppose the change in Gibbs free energy is greater than zero (ΔG > 0), then the reaction is nonspontaneous and endergonic.
Suppose the change in Gibbs free energy is less than zero (ΔG < 0), then the reaction is spontaneous and exergonic.
Suppose the change in Gibbs free energy is equal to zero (ΔG = 0), then the reaction is at equilibrium condition.
There are some important key points to be remembered regarding Gibbs free energy such as:
According to the second law of thermodynamics, the entropy of the universe always increases for a spontaneous process and it can never be equal to zero.
The change in Gibbs free energy (ΔG) determines the direction and extent of chemical change.
The change in Gibbs free energy (ΔG) is useful only for reactions in which the temperature and pressure remain constant (i.e., it is in good agreement with the isothermal and isobaric process). The system is usually open to the atmosphere (constant pressure) and we initiate and terminate the process at room temperature (after any heat we have supplied or which is released by the reaction has dissipated).
Standard Gibbs free energy is often used as the single master variable that determines whether a given chemical change is thermodynamically possible. Thus, if the change in free energy of the reactants is more than that of the products, the entropy of the world will increase when the reaction takes place as written, and so the reaction will tend to take place spontaneously.
ΔSuniverse = ΔSsystem + ΔSsurroundings
If the change in Gibbs free energy is negative, the process will occur spontaneously and is referred to as exergonic.
Therefore spontaneity of the reaction is dependent on the temperature of the system (Gibbs free energy spontaneous).
Even though the change in Gibbs free energy is temperature-dependent, we assume the change in enthalpy ∆H and the change in entropy ∆S independent of temperature when there is no phase change in the reaction. So if we know the change in enthalpy ∆H and the change in entropy ∆S, we can calculate the change in Gibbs free energy ∆G at any temperature.
Relationship Between Free Energy and Equilibrium Constant
The change in Gibbs free energy of the thermodynamic reaction in any state, ΔG (at equilibrium) is related to the standard free energy change of the reaction, ΔG° (that is equal to the difference in the free energies of creation of the products and reactants both in their standard states)
According to the equation:
ΔG = ΔG° + RT In Q
Where,
Q- The reaction quotient.
∆G = 0 and Q become adequate to the constant. Hence the equation becomes,
G0 = -RT ln Keq
G0 = -2.303 RT log Keq
Where,
R = gas constant = 8.31 J mol-1 K-1 or 0.008314 kJ mol-1 K-1
T is the temperature on the Kelvin scale
In any reversible reaction, the free energy of the reaction mixture is less than the free energy of reactants also as products. Hence, Gibbs free energy decreases whether we start from reactants or products i.e, ∆G is -ve in both backward and the forward reactions.
Relationship Between Gibbs Free Energy and EMF of a Cell
In the case of galvanic cells, Gibbs energy change ΔG is said to be the trade done by the cell.
ΔG = -nFEcell
Where,
n = no. of moles of electrons involved
F = the Faraday constant
E = emf of the cell
We know that 1 Faraday = 96500 coulombs.
Did You Know?
We know that both the enthalpy of the system and the Gibbs free energy are the thermodynamic potentials, and one of the unique facts is that even the unit of ∆G is the same as that of ∆H.
The tesla free energy is modern free energy, though it is named free energy it is not free, it requires components. Usually found in a free electricity generator or free energy motor.
A free energy generator magnet follows a mechanism that generates electrical energy using the neodymium magnet theory. There are various sizes of generators, and one kind of generator that produces electrical energy is the free energy generator.
FAQs on Gibbs Free Energy
1. What is Gibbs free energy in simple terms?
In simple terms, Gibbs free energy (G) is the maximum amount of energy available from a chemical reaction that can be used to do useful work. It helps predict whether a reaction will happen on its own (spontaneously) under conditions of constant temperature and pressure.
2. What is the formula for the change in Gibbs free energy and what do its components represent?
The formula for the change in Gibbs free energy is the Gibbs-Helmholtz equation: ΔG = ΔH - TΔS. Each component is crucial for understanding a reaction's feasibility:
- ΔG is the change in Gibbs free energy.
- ΔH is the change in enthalpy, which is the total heat content of the system.
- T is the absolute temperature in Kelvin.
- ΔS is the change in entropy, which is a measure of the disorder or randomness in the system.
3. How do you determine if a reaction is spontaneous using Gibbs free energy?
The sign of the change in Gibbs free energy (ΔG) for a process at constant temperature and pressure determines its spontaneity:
- If ΔG is negative (< 0), the reaction is spontaneous and can proceed on its own. Such reactions are called exergonic.
- If ΔG is positive (> 0), the reaction is non-spontaneous and requires energy input to occur. These are endergonic reactions.
- If ΔG is zero (= 0), the system is at equilibrium, and there is no net change in the forward or reverse direction.
4. What is the standard unit of Gibbs free energy?
The standard SI unit for Gibbs free energy is Joules (J) per mole (mol). Because reaction energies are often large, it is commonly expressed in Kilojoules per mole (kJ/mol). This unit is the same as that used for enthalpy and work.
5. How does Gibbs free energy relate to the work done by an electrochemical cell?
For an electrochemical cell, such as a galvanic cell, the change in Gibbs free energy represents the maximum electrical work the cell can perform. The relationship is given by the formula ΔG = -nFEcell, where:
- n is the number of moles of electrons transferred in the reaction.
- F is the Faraday constant (approximately 96,500 C/mol).
- Ecell is the electromotive force (emf) or cell potential.
A positive Ecell results in a negative ΔG, indicating a spontaneous reaction that can generate electrical energy.
6. Why is it called 'free' energy? Does this mean the energy is available at no cost?
The term 'free' in Gibbs free energy does not mean it costs nothing. It refers to the portion of a system's total energy (enthalpy) that is 'free' or available to be converted into useful work. The other part of the energy, represented by the TΔS term, is the energy that is unavailable because it is tied up in maintaining the system's entropy or disorder. So, it's the 'useful' energy, not 'gratis' energy.
7. How are the standard Gibbs free energy change (ΔG°) and the equilibrium constant (K) related?
The standard Gibbs free energy change (ΔG°) and the equilibrium constant (K) are linked by the important equation: ΔG° = -RT ln(K). This relationship signifies that:
- If K > 1, ln(K) is positive, making ΔG° negative. This means the reaction spontaneously favours the formation of products at standard conditions.
- If K < 1, ln(K) is negative, making ΔG° positive. This indicates that the reactants are favoured at equilibrium.
- If K = 1, ln(K) is zero, and ΔG° is zero, meaning the reaction is at equilibrium with equal concentrations of reactants and products under standard conditions.
8. Can a reaction that absorbs heat (endothermic) still be spontaneous? How does Gibbs free energy explain this?
Yes, an endothermic reaction (where ΔH is positive) can be spontaneous. This is possible if the reaction leads to a large increase in disorder (a large positive ΔS). According to the equation ΔG = ΔH - TΔS, the term -TΔS can become a large negative number, especially at high temperatures. If this negative entropy term is larger in magnitude than the positive enthalpy term, the overall ΔG will be negative, making the reaction spontaneous. A common example is the melting of ice above 0°C.

















