The Beautiful Bridge Between Kinetics and Thermodynamics
Have you ever wondered how the microscopic dance of molecules—their collisions, their energy barriers, their frantic movements—translates into the grand, sweeping laws of thermodynamics? This problem is a perfect, elegant example of exactly that. We are going to build a bridge from the Arrhenius equation of chemical kinetics straight into the heart of Gibbs Free Energy.
Imagine you are standing at the foot of a mountain. To get to the valley on the other side, you have to climb over the peak. In chemistry, that peak is the activation energy.
Analyzing the Setup
The problem gives us a reversible reaction:
A(g)+B(g)⇌AB(g)
We are told a crucial piece of information: the activation energy of the backward reaction (
Eab) exceeds that of the forward reaction (
Eaf) by
2RT. Mathematically, this is:
Eab−Eaf=2RT
What does this mean physically? If it takes more energy to go backward than to go forward, the products must be at a lower energy state than the reactants. This is an exothermic reaction! The difference between these two activation energies is exactly the enthalpy change of the reaction, ΔH.
The Master Equation
Equilibrium Constant
Now, how do we connect these kinetic parameters to equilibrium? At equilibrium, the rate of the forward reaction equals the rate of the backward reaction. This fundamental balance gives us the equilibrium constant
Keq as the ratio of the forward rate constant to the backward rate constant:
Keq=kbkf
This is where the magic happens. We bring in the Arrhenius equation,
k=Ae−Ea/RT, and substitute it for both rate constants:
Keq=Abe−Eab/RTAfe−Eaf/RT
Let's group the terms to make it cleaner:
Keq=(AbAf)e(Eab−Eaf)/RT
Plugging in the Magic Numbers
The problem generously hands us the pieces of this puzzle. We know the pre-exponential factor of the forward reaction is 4 times that of the reverse, so
AbAf=4. We also know the exponent numerator
Eab−Eaf=2RT. Let's substitute these in:
Keq=4⋅e2RT/RT
Keq=4e2
Look at how beautifully the RT terms cancelled out in the exponent! We now have a clean, exact value for our equilibrium constant.
The Final Calculation
Gibbs Free Energy
We have arrived at the thermodynamic side of the bridge. The standard Gibbs Free Energy,
ΔG∘, is intimately tied to the equilibrium constant by the famous equation:
ΔG∘=−RTlnKeq
Let's substitute our
Keq:
ΔG∘=−RTln(4e2)
Here is where many students make a silly mistake. Don't rush the logarithm! Use the properties of logs to expand it carefully:
ln(ab)=ln(a)+ln(b).
ln(4e2)=ln(4)+ln(e2)
ln(4e2)=2ln(2)+2
Now, we plug in the given values:
ln(2)=0.7 and
RT=2500 J mol−1.
ln(4e2)=2(0.7)+2=1.4+2=3.4
Finally, calculate
ΔG∘:
ΔG∘=−2500×3.4=−8500 J mol−1
The negative sign tells us the reaction is spontaneous in the forward direction under standard conditions. However, the question specifically asks for the absolute value of ΔG∘.
Therefore, our final answer is 8500.
Take a moment to appreciate what we just did. We took microscopic collision parameters and derived a macroscopic thermodynamic property. That is the true power of physical chemistry!