Free Energy
The second law of thermodynamics can be used to predict spontaneity.
But measurements on the surroundings are seldom made.
This limits the use of the second law of thermodynamics.
It is convenient to have a thermodynamic function that focuses on just the system and predicts spontaneity.
The changes in Gibbs free energy (ΔG) or simply change in free energy allow us to predict spontaneity by focusing on the system only.
ΔG = ΔH – TΔS
The sign of ΔG indicates if a reaction will be spontaneous or not.
If ΔG < 0, the reaction is spontaneous in the forward direction.
If ΔG > 0, the reaction is nonspontaneous in the forward direction
If ΔG = 0, the system is at equilibrium
Spontaneous reactions, those with –ΔG, generally have:
ΔH < 0
Exothermic reaction.
A negative ΔH will contribute to a negative ΔG.
ΔS > 0
A positive ΔS will contribute to a negative ΔG.
Note that a reaction can still be spontaneous (have a –ΔG) when ΔH is positive or ΔS is negative, but not both.
Also note that there is a temperature dependence.
To calculate the temperature at which the spontaneity of a reaction changes from …
Spontaneous to nonspontaneous
Or nonspontaneous to spontaneous
Find the temperature at which ΔG = 0
ΔG = 0 = ΔH – TΔS
T = ΔH / ΔS
This is the temperature at which ΔG = 0 and, by definition, the system is at equilibrium.
Although the Change in Gibbs Free Energy equation is valid under all conditions, we will most often apply it at standard conditions.
Standard conditions:
Under standard conditions, ΔG° = ΔH° – TΔS°
Pay attention to J vs. kJ in calculations!
Standard free energy of formation (∆G°f): the free energy change for the formation of one mole of a substance from its elements in their standard state at 1 bar and 25 °C.
ΔG° = ΣnΔG° f (products) – ΣnΔG° f (reactants)
This equation only works for calculating ∆G° of a reaction at the temperature for which the values of ∆G°f are tabulated, which is 298 K.
ΔG°f for any element in its most stable form at standard conditions is defined as zero. ( Just as is the case for ΔHf )
But S° for an element is NOT zero!!
For a reaction to be spontaneous, K must be greater than 1.
But “spontaneous” here means that the products are favored when ALL components are 1 M or 1 atm.
It should be clear that if K>1, (favored) then ΔG° must be -
As with enthalpy, free energy changes for reactions are additive
If Reaction 3 = Reaction 1 + Reaction 2 then, ΔG3 = ΔG1 + ΔG2
Also keep in mind that if a reaction is reversed, then the sign on ΔG is also reversed.
If a reaction is multiplied by a factor of “n,” then ΔG is also multiplied by a factor of “n.”
The second law of thermodynamics can be used to predict spontaneity.
But measurements on the surroundings are seldom made.
This limits the use of the second law of thermodynamics.
It is convenient to have a thermodynamic function that focuses on just the system and predicts spontaneity.
The changes in Gibbs free energy (ΔG) or simply change in free energy allow us to predict spontaneity by focusing on the system only.
ΔG = ΔH – TΔS
The sign of ΔG indicates if a reaction will be spontaneous or not.
If ΔG < 0, the reaction is spontaneous in the forward direction.
If ΔG > 0, the reaction is nonspontaneous in the forward direction
If ΔG = 0, the system is at equilibrium
Spontaneous reactions, those with –ΔG, generally have:
ΔH < 0
Exothermic reaction.
A negative ΔH will contribute to a negative ΔG.
ΔS > 0
A positive ΔS will contribute to a negative ΔG.
Note that a reaction can still be spontaneous (have a –ΔG) when ΔH is positive or ΔS is negative, but not both.
Also note that there is a temperature dependence.
To calculate the temperature at which the spontaneity of a reaction changes from …
Spontaneous to nonspontaneous
Or nonspontaneous to spontaneous
Find the temperature at which ΔG = 0
ΔG = 0 = ΔH – TΔS
T = ΔH / ΔS
This is the temperature at which ΔG = 0 and, by definition, the system is at equilibrium.
Although the Change in Gibbs Free Energy equation is valid under all conditions, we will most often apply it at standard conditions.
Standard conditions:
Under standard conditions, ΔG° = ΔH° – TΔS°
Pay attention to J vs. kJ in calculations!
Standard free energy of formation (∆G°f): the free energy change for the formation of one mole of a substance from its elements in their standard state at 1 bar and 25 °C.
ΔG° = ΣnΔG° f (products) – ΣnΔG° f (reactants)
This equation only works for calculating ∆G° of a reaction at the temperature for which the values of ∆G°f are tabulated, which is 298 K.
ΔG°f for any element in its most stable form at standard conditions is defined as zero. ( Just as is the case for ΔHf )
But S° for an element is NOT zero!!
For a reaction to be spontaneous, K must be greater than 1.
But “spontaneous” here means that the products are favored when ALL components are 1 M or 1 atm.
It should be clear that if K>1, (favored) then ΔG° must be -
As with enthalpy, free energy changes for reactions are additive
If Reaction 3 = Reaction 1 + Reaction 2 then, ΔG3 = ΔG1 + ΔG2
Also keep in mind that if a reaction is reversed, then the sign on ΔG is also reversed.
If a reaction is multiplied by a factor of “n,” then ΔG is also multiplied by a factor of “n.”