In a practical and frequently used form of Gibbs free energy change equation, ΔG is calculated from a set values that can be measured by scientists: the enthalpy and entropy changes of a reaction, together with the temperature at which the reaction takes place.
ΔG=ΔH−TΔS
Let’s take a step back and look at each component of this equation.
By looking at ∆H and ∆S, we can tell whether a reaction will be spontaneous, non-spontaneous, or spontaneous only at certain temperatures.
If a reaction both releases heat and increases entropy, it will always be spontaneous (have a negative ∆G), regardless of temperature.
Similarly, a reaction that both absorbs heat and decreases entropy will be non-spontaneous (positive ∆G) at all temperatures.
Some reactions, however, have a mix of favorable and unfavorable properties (releasing heat but decreasing entropy, or absorbing heat but increasing entropy). The ∆G and spontaneity of these reactions will depend on temperature, as summarized in the table at right.
[Why can these terms predict spontaneity?]
At this point, you may be wondering why this set of terms (∆H, ∆S, and T) can predict reaction spontaneity.
According to the Second Law of Thermodynamics, a reaction will be spontaneous only if it increases the overall entropy of the universe. So, why mess around with ΔH and T?
In the ΔG equation shown above, ΔS (the entropy change of the system) is clearly entropy-related, and an increase in entropy favors spontaneity.
However, ΔH and T are also entropy-related, albeit in an indirect way. Released heat can increase (and absorbed heat can decrease) the entropy of the surroundings, and the magnitude of the change depends on temperature. Thus, all three terms of the ΔG equation actually relate to a reaction’s effect on the entropy of the universe.
For a more thorough and rigorous explanation of the relationship between ∆G and the entropy of the universe, check out this video on thermodynamics.