Thermochemical equations and their rules are fundamental for understanding energy changes in chemical reactions. By using these equations, we can determine whether a reaction absorbs or releases heat. Hess's Law further aids in calculating the enthalpy changes for complex reactions by breaking them down into simpler, more manageable steps, making it an invaluable tool in thermochemistry.
A thermochemical equation represents a balanced chemical reaction along with the physical states of all reactants and products, as well as the heat change involved in the reaction. This equation provides information about the amount of energy absorbed or released during a chemical reaction.
Here is an example of a Thermochemical Equation:
CH4 (g) + 2O2 (g) → CO2 (g) + 2H2O (l) + 890.4 kJ
A reaction that releases heat energy into the surroundings.
Example: Combustion of Ethanol
C2H5OH(ℓ) + 3O2(g) → 2CO2(g) + 3H2O (ℓ) ΔrHO=−1367 kJ/mol
The negative sign indicates that 1367 kJ of heat is released per mole of ethanol combusted.
Alternate Forms of the Thermochemical Equation:
C2H5OH(ℓ) + 3O2(g) → 2CO2(g) + 3H2O(ℓ) + 1367 kJ
C2H5OH (ℓ) + 3O2(g) −1367 kJ → 2CO2(g) + 3H2O (ℓ)
These different representations all convey that the reaction releases 1367 kJ of energy.
A reaction that absorbs heat energy from the surroundings.
Example: Dissolution of Copper(II) Sulfate Pentahydrate
CuSO4⋅5H2O(s) + aq → CuSO4 (aq) ΔsolH=11.71 kJ
The positive sign indicates that 11.71 kJ of heat is absorbed during the dissolution.
Alternate Forms of the Thermochemical Equation:
CuSO4⋅5H2O (s) + aq → CuSO4(aq) − 11.71 kJ
CuSO4⋅5H2O (s) + aq + 11.71kJ → CuSO4(aq)
These representations show that 11.71 kJ of energy is absorbed during the process.
Important Points:
These coefficients define the proportion in which reactants combine and products are formed, and they are crucial for calculating the heat change per mole of reaction.
Thermochemical equations provide information about the heat changes associated with chemical reactions. Understanding these equations and their rules is essential for predicting the energy requirements or releases during reactions.
Rule #1: Proportionality of Enthalpy Change (ΔH)
Example Reactions:
Rule #2: Reversibility of Enthalpy Change
Example Reactions:
Rule #3: Independence of Reaction Path
Hess’s Law is useful for calculating ΔH for reactions that are difficult to carry out directly. It states that the total enthalpy change for a reaction is the sum of the enthalpy changes for each step of the reaction pathway.
Example:
Target Reaction: C(s) + 12O2(g) → CO(g); ΔH1=?
Given Reactions:
Steps to Calculate ΔH1:
C(s) + O2(g) → CO2(g); ΔH3 = −393.5 kJ
CO2(g) → CO(g) + 12O2(g); −ΔH2 = +283.0 kJ
C(s) + 12O2(g) → CO(g); ΔH1=−393.5 kJ + 283.0 kJ
ΔH1=−110.5kJ
Thus, the enthalpy change for the reaction C(s)+12O2(g) → CO(g) is ΔH1=−110.5 kJ
(Session 2025 - 26)