Warm up and recall
Three quick questions from earlier lessons. Pulling old material back to mind before you learn something new makes the new material stick better, so this is not busywork.
Practise this lesson
Four printable worksheets that build from the foundations up to exam-style questions, start at whatever level suits you.
Where this lesson fits
Lesson question: how can you calculate the enthalpy change of almost any reaction from a single table of numbers, without ever running an experiment?
- 1Define ΔH°f. The standard enthalpy of formation is the enthalpy change when 1 mole of a compound forms from its elements in their standard states.
- 2Note elements = 0. The ΔH°f of any element in its standard state is defined as zero, so it drops out of the sum.
- 3Apply the formula. ΔH°rxn = ΣΔH°f(products) − ΣΔH°f(reactants), each value scaled by its coefficient.
Quick prerequisite: you need the ΔH sign convention from Lesson 1 (negative = exothermic, positive = endothermic). Because enthalpy is a state function, this method is really a Hess's-Law cycle, which Lesson 8 develops in full. If the sign convention is shaky, start with the Supported route later in this lesson. Syllabus reference: investigate Hess's Law in quantifying the enthalpy change for a stepped reaction using standard enthalpy change data and bond energy data (ACSCH037).
Know what matters most
Must know
- ΔH°f = enthalpy change when 1 mol of a compound forms from its elements in their standard states
- ΔH°f of any element in its standard state = 0 kJ mol⁻¹
- ΔH°rxn = ΣΔH°f(products) − ΣΔH°f(reactants)
Should know
- Standard state = the most stable physical form of an element at 25°C and 100 kPa
- How to read a ΔH°f data table and scale each value by its stoichiometric coefficient
- Why this method is more accurate than the bond energy method
Going deeper
- Why standard conditions (298 K, 100 kPa) matter and are always specified
- Why the ΔH°f method is itself a Hess cycle (state function)
Warm up and recall
A rocket engineer in 1969 needs to calculate how much energy N₂H₄ releases when it burns in the Apollo lunar module descent engine. They cannot run a calorimetry experiment on a rocket, the conditions are too extreme and the stakes too high. Instead, they open a thermochemical data table.
The table lists the standard enthalpy of formation of each compound involved: how much energy was absorbed or released when that compound was made from its elements under standard conditions. With just those numbers and the balanced equation, the engineer calculates ΔH precisely.
Before this lesson: In Lesson 6, you calculated ΔH using average bond energies. What limitations did that method have? How might tabulated formation enthalpies overcome them? Write your thinking before the lesson explains it.
What you'll master, and the words for it
Key Facts
- ΔH°f = enthalpy change when 1 mol of compound forms from elements in standard states at 25°C, 100 kPa
- ΔH°f of any element in its standard state = 0 kJ mol⁻¹
- Formula: ΔH°rxn = ΣΔH°f(products) − ΣΔH°f(reactants)
Concepts
- Why ΔH°f of elements = 0 (by definition, no change forming an element from itself)
- Why this method is more accurate than bond energies (experimental data, actual states)
- The key difference in formula direction from the bond energy method
Skills
- Write a formation equation for a given compound (1 mol product, elements as reactants)
- Calculate ΔH°rxn from a data table using products minus reactants
- Scale ΔH°f values by stoichiometric coefficients correctly