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1.3 Electron configurations

Syllabus
First assessment 2025
Topic
1.3
Level
SL

Emission Spectra

An emission photon is released when an electron falls from a higher energy state to a lower energy state. Absorption moves an electron upward and requires photon energy.

Spectrum What it contains Why
Line spectrum Specific wavelengths, frequencies, energies, or colours Electrons occupy discrete energy levels, so only particular transitions occur
Continuous spectrum A continuous range across the relevant values The radiation spans the range rather than appearing as separated lines

Across electromagnetic radiation, shorter wavelength means higher frequency, and higher frequency means higher photon energy. Explain the electron direction and photon exchange when distinguishing absorption from emission.

Read every spectral transition in two directions: absorption raises an electron by ΔE, while a downward transition emits a photon with ΔE = hf = hc/λ. A shorter-wavelength line therefore represents a larger energy gap, not a higher line intensity.

Orient the spectrum before comparing lines: radio → microwave → infrared → visible → ultraviolet → X-ray → gamma is increasing frequency and photon energy, and decreasing wavelength. Within visible light, red has longer wavelength and lower photon energy than violet.

Explaining Absorption and Emission

Assessment in practice

2 marks in each selected direct example marks
How it is assessed

Structured questions ask learners to distinguish absorption from emission by the direction of electron movement and photon transfer, and to distinguish continuous spectra from line spectra by their wavelength or frequency coverage.

Command terms

distinguish

What earns marks

State the direction of the electron transition and whether a photon is absorbed or emitted, then classify a continuous spectrum as spanning the range and a line spectrum as containing only specific wavelengths, frequencies, energies, or colours.

Watch for

Reversing absorption and emission, or describing a line spectrum as continuous rather than as discrete allowed wavelengths or frequencies.

Representative question

Question 1

[Maximum number: 2]

Distinguish between the processes within the atom that give rise to absorption and emission spectra.

Absorption spectra:

Emission spectra:

Hydrogen's Line Spectrum

Hydrogen's emission spectrum contains discrete lines because electrons occupy discrete energy levels. Each line corresponds to a downward transition and the emitted photon's energy equals the energy difference between the levels.

Transition ending at Region identified in the study guide
n = 1 ultraviolet
n = 2 visible
n = 3 infrared

At higher energy, the levels become closer together, so the lines converge. The names of the series are not required.

Use the presence of separate lines as evidence for discrete levels, and use convergence at higher energy or frequency as evidence that the level spacing becomes smaller.

Compare lines by their energy gaps. Transitions ending at n = 2 form the visible series, and lines crowd together as the starting level rises because adjacent high-n levels are closer in energy. The convergence limit represents removal of the electron, not one more bound-state transition.

Interpreting Hydrogen Emission Lines

Assessment in practice

2–3 marks in the two selected direct examples marks
How it is assessed

Structured questions ask learners to describe hydrogen's discrete line spectrum and explain how each line corresponds to an electron energy difference and how the lines converge at higher energy.

Command terms

describe / explain

What earns marks

Identify discrete lines or specific wavelengths/frequencies, connect each line to a downward transition and its energy difference, and state that energy levels become closer together at higher energy, producing convergence.

Watch for

Calling the hydrogen spectrum continuous, reversing the downward emission transition, or placing convergence at lower rather than higher energy or frequency.

Representative question

Question 1

[Maximum number: 3]

Explain how this spectrum is related to the electron energy levels in a hydrogen atom.

Main Energy-Level Capacity

A main energy level, or shell, is identified by the principal quantum number n = 1, 2, 3, and so on.

maximumelectrons=2n2maximum electrons = 2n²

n Maximum electrons
1 2
2 8
3 18
4 32

Substitute the stated n value into 2n²; do not confuse the shell number with the capacity.

For n = 3, the theoretical capacity is 2(3²) = 18 electrons. This is a capacity, not a claim that every third shell is full: the actual occupancy depends on the atom and the relative energies of available sublevels.

Calculating Shell Capacity

Assessment in practice

1 mark in each selected direct example marks
How it is assessed

Short multiple-choice questions ask learners to calculate the maximum electron capacity for a stated main energy level using the 2n² rule.

Command terms

state

What earns marks

Substitute the stated integer n into 2n² and select or state the resulting maximum electron count.

Watch for

Using n² instead of 2n², or confusing a main energy level's total capacity with the capacity of one subshell or orbital.

Representative question

Question 1

[Maximum number: 1]

What is the maximum number of electrons that can occupy the n=3 main energy level?

A

3

B

8

C

18

D

28

Sublevels, Orbitals, and Blocks

A main energy level contains only the sublevels allowed by its principal quantum number: n = 1 has s; n = 2 has s and p; n = 3 has s, p and d; and n = 4 can include s, p, d and f. Within one main level the sublevels rise in energy s < p < d < f, while the filling order across different levels can interleave, as the next card makes explicit. Each sublevel contains a fixed number of orbitals.

Sublevel Number of orbitals Maximum electrons Assessed shape evidence Periodic-table block
s 1 2 spherical s block
p 3 6 three dumbbell orbitals with different orientations p block
d 5 10 shape detail not required here d block
f 7 14 shape detail not required here f block

The block is identified by the subshell being filled; sublevel capacity is not the same as actual occupancy.

For recognition questions, keep the hierarchy clear: main energy level → sublevel → orbital. The s and p shapes are the explicitly required shape evidence here.

Use the hierarchy as a classification test: a p sublevel contains three orbitals, and each orbital can hold two electrons. An orbital describes a probability region with a characteristic shape; it is not a circular route travelled by an electron.

Recognising Orbital Shapes

Assessment in practice

1–2 marks in the two selected direct examples marks
How it is assessed

Questions ask students to recognize or sketch the characteristic s-orbital sphere and p-orbital dumbbell, with labels where required.

Command terms

sketch

What earns marks

Match each orbital label to its shape and show the p-orbital lobes with the correct orientation; keep the orbital-shape model distinct from the number of orbitals in a sublevel and from the periodic-table block label.

Watch for

Drawing an s orbital as a dumbbell or a p orbital as a sphere

Representative question

Question 1

[Maximum number: 2]

Sketch the shapes of two different orbital types in the second energy level and label each orbital.

Electron Configurations and Spin

Aufbau fills lower-energy orbitals first. Pauli limits an orbital to two electrons with opposite spins. Hund's rule places electrons singly in degenerate orbitals before pairing.

Representation Use
Full configuration Show the complete filling sequence
Condensed configuration Replace the inner electrons with a noble-gas core
Orbital-box diagram Show orbital occupancy and opposite-spin pairing

For ions, remove 4s electrons before 3d electrons. The exceptions in scope are Cr: [Ar] 4s1 3d5 and Cu: [Ar] 4s1 3d10.

Check total electrons, obey the filling order, apply Hund and Pauli in each sublevel, and treat the Cr/Cu exceptions explicitly rather than forcing the naive pattern.

Build an orbital diagram by checking electron total, energy order, single occupation of equal-energy orbitals, then opposite-spin pairing. For transition-metal ions remove 4s electrons before 3d, and verify Cr and Cu against the stated exceptions rather than forcing the simple filling pattern.

Worked ion check: Fe has 26 electrons and condensed configuration [Ar] 4s² 3d⁶. To form Fe³⁺, remove the two electrons from the highest principal level, 4s, before removing one 3d electron, giving [Ar] 3d⁵. The final superscripts total 23 electrons, matching 26 − 3.

Constructing Electron Configurations

Assessment in practice

1–2 marks in the two selected direct examples marks
How it is assessed

Questions ask students to draw and label a ground-state orbital diagram or select/configure an atom using the filling rules and the Cr/Cu exceptions.

Command terms

draw

What earns marks

Fill orbitals in the stated energy order, place one electron in each degenerate orbital before pairing, pair only opposite spins, remove 4s electrons before 3d for transition-metal ions, and use the accepted Cr/Cu exception configurations.

Watch for

Pairing electrons in a p or d sublevel before singly occupying equivalent orbitals

Representative question

Question 1

[Maximum number: 2]

Draw the orbital diagram of the phosphorus atom in the ground state by adding, filling and labelling the orbitals. Use section 7 of the data booklet.

2s

1s

Electron Configurations Summary

Retrieve the chain: emission lines reveal discrete levels; capacities, sublevels, orbitals, and spin rules build configurations; first and successive ionization energies then reveal how electrons are held and arranged.

When checking an answer, ask: Did I link a line to a transition? Did I use 2n² and the filling rules? Did I explain an ionization trend or count electrons before a successive-IE jump?

ConceptIB Chemistry SL