Question
Question: Solid \(Ca{{\left( HC{{O}_{3}} \right)}_{2}}\) decomposes as \[Ca{{\left( HC{{O}_{3}} \right)}_{2}...
Solid Ca(HCO3)2 decomposes as
Ca(HCO3)2(s)⇌CaCO3(s)+CO2(g)+H2O(g)
If the total pressure is 0.2 bar at 420 K, what is the standard free energy change for the given reaction(ΔrGo)?
(A) 840 KJ/mol
(B) 3.86 KJ/mol
(C) 6.98 KJ/mol
(D) 16.083 KJ/mol
Solution
When calcium bicarbonate is subjected to heating it is decomposed to give calcium carbonate, carbon dioxide and water. The calcium bicarbonate is soluble in water whereas calcium carbonate is insoluble in water.
Complete step by step solution:
- By looking at the stoichiometry of the reaction of decomposition of Ca(HCO3)2, we can assume that the partial pressure of carbon dioxide is equal to the partial pressure of water. And hence we can write as follows
PCO2=PH2O
It’s given that the total pressure is 0.2 bar. Thus we can write as follows
PCO2+PH2O=0.2bar
We can modify the above relation as follows
2PCO2=2PH2O=0.2bar
At equilibrium the relation becomes,
PCO2=PH2O=0.1bar
Keq=PCO2×PH2O=0.1bar2
Keq=0.01bar2
We are asked to find the ΔrGo value. The relation between Gibbs energy and standard free energy change can be written as follows
ΔG=ΔGo+RTlnKeq
At equilibrium ΔG is zero and the above relation can be modified as follows
ΔGo=−RTlnKeq
As we know R is the universal gas constant and its value is 8.314Jmol−1K−1. T is the temperature in kelvin and the value is given in the question as 420 K. We have found the value of Keq as 0.01. Let’s substitute this values in the above equation
ΔGo=−8.314×420×ln(0.01)=16081.6688Jmol−1
We know that 1J=10−3KJ. Thus by converting the above values in joules into kilojoules we get a follows
ΔrGo=16.082KJ/mol
Thus the standard free energy change for the given reaction ΔrGo is 16.083 KJ/mol.
Therefore the answer is option (D) 16.083 KJ/mol
Note: The standard-state free energy of formation can be defined as the variation in free energy which happens when a compound is formed from its elements at standard-state conditions in their most thermodynamically stable states. It can also be defined as the difference between the free energies of constituent elements and the free energy of its substance at standard-state condition.