Analyzing the Setup
Let's dive into a classic problem from Chemical Thermodynamics that beautifully connects the standard free energy of a reaction with its equilibrium constant. We are given the reaction:
We are provided with the standard free energy of formation for NO(g), which is 86.6 kJ/mol, and the equilibrium constant Kp=1.6×1012 at a temperature of 298 K. Our goal is to find the standard free energy of formation for the product, NO2(g).
To visualize this, imagine a thermodynamic cycle. At the base, we have our constituent elements in their standard states: N2(g) and O2(g). These elements can either form our reactants (2NO+O2) or directly form our products (2NO2). The difference in energy between these two pathways is exactly the standard free energy of the reaction, ΔGr∘.
The Master Equations
There are two fundamental equations we need to bridge together. First, the standard free energy of the reaction can be calculated from the formation energies of the individual species:
ΔGr∘=∑ΔGf∘(products)−∑ΔGf∘(reactants)
Applying this to our specific reaction, and remembering to multiply by the stoichiometric coefficients, we get:
ΔGr∘=2ΔGf∘(NO2)−[2ΔGf∘(NO)+ΔGf∘(O2)]
Second, we know that the standard free energy of a reaction is intimately linked to the equilibrium constant Kp through the isotherm equation:
Equating and Substituting
By equating these two expressions for ΔGr∘, we create a powerful equation that contains our unknown variable:
−RTlnKp=2ΔGf∘(NO2)−[2ΔGf∘(NO)+ΔGf∘(O2)]
Now, let's substitute the known values. Here is where we must be extremely careful with units! The gas constant R is typically expressed in Joules, but our formation energy for NO is given in kilojoules (86.6 kJ/mol). We must convert this to 86600 J/mol. Furthermore, remember that the standard free energy of formation for an element in its most stable standard state, like O2(g), is exactly zero.
−R(298)ln(1.6×1012)=2ΔGf∘(NO2)−[2(86600)+0]
Final Calculation
Our final task is simple algebraic rearrangement. We want to isolate the term 2ΔGf∘(NO2). We do this by moving the reactant energy term to the left side of the equation:
2ΔGf∘(NO2)=2(86600)−R(298)ln(1.6×1012)
Finally, to find the formation energy for a single mole of NO2, we divide the entire right side by 2 (which is the same as multiplying by 0.5):
ΔGf∘(NO2)=0.5[2×86600−R(298)ln(1.6×1012)]
This perfectly matches option (d). The beauty of this problem lies in the seamless integration of Hess's Law principles with chemical equilibrium, reminding us that thermodynamics is a perfectly consistent logical framework.