Electrons, energy levels and ionisation energy

Section: 1 Atomic Structure  |  Syllabus: Cambridge AS Level Chemistry (9701)

Shells, Sub-shells and Orbitals

Shell (Principal Energy Level) A main energy level occupied by electrons, described by the principal quantum number n (n = 1, 2, 3...). Higher n means further from the nucleus and higher energy. Sub-shell A subdivision of a shell, labelled s, p, d or f. Each shell contains one or more sub-shells. Orbital A region of space around the nucleus that can hold a maximum of 2 electrons (with opposite spins). Each orbital has a specific shape and energy. Ground State The lowest energy electronic configuration of an atom or ion, where electrons fill the lowest available energy levels first.

Sub-shells: Orbitals and Electron Capacity

Principal Quantum Number (n) Sub-shell Number of Orbitals Max Electrons in Sub-shell Max Electrons in Shell
1 1s 1 2 2
2 2s 1 2 8
2p 3 6
3 3s 1 2 18
3p 3 6
3d 5 10
4 4s 1 2 (32)
4p 3 6
Key Rule

Each orbital holds a maximum of 2 electrons with opposite spins (↑↓). An s sub-shell has 1 orbital, a p sub-shell has 3 orbitals, and a d sub-shell has 5 orbitals.

Order of Increasing Energy (Aufbau Principle)

Electrons fill sub-shells in order of increasing energy. The order is:

Important Exception

The 4s sub-shell fills before the 3d because it is at a slightly lower energy level. However, when a transition metal ion forms, 4s electrons are lost first - because once the 3d is occupied, the 3d energy falls below 4s.

This filling order can be remembered using the diagonal arrow diagram (Aufbau diagram): draw sub-shells in a grid and follow diagonal arrows from top right to bottom left.

Figure 1.8: Aufbau Filling Order Diagram

(Grid with sub-shells listed: 1s, 2s 2p, 3s 3p 3d, 4s 4p 4d 4f. Diagonal arrows running from top-right to bottom-left showing the filling order: 1s → 2s → 2p → 3s → 3p → 4s → 3d → 4p. Highlight that 4s is filled before 3d.)

Electronic Configurations

Two conventions are used to express electronic configurations:

Full notation

Write all sub-shells explicitly with superscripts for electron numbers:

Examples

Na (Z=11): 1s² 2s² 2p⁶ 3s¹

Cl (Z=17): 1s² 2s² 2p⁶ 3s² 3p⁵

Fe (Z=26): 1s² 2s² 2p⁶ 3s² 3p⁶ 3d⁶ 4s²

Shorthand (noble gas core) notation

Use the preceding noble gas symbol in square brackets to replace the core configuration:

Examples

Na: [Ne] 3s¹

Cl: [Ne] 3s² 3p⁵

Fe: [Ar] 3d⁶ 4s²

Ions

Examples: Iron ions

Fe²⁺: remove 2 electrons from 4s → [Ar] 3d⁶

Fe³⁺: remove 2 from 4s, 1 from 3d → [Ar] 3d⁵

Electrons in Boxes Notation

Each box represents one orbital. Electrons are shown as arrows (↑ = spin up, ↓ = spin down).

Two key rules apply when filling orbitals in the same sub-shell:

Example: Carbon (1s² 2s² 2p²)

1s: [↑↓] 2s: [↑↓] 2p: [↑][↑][ ]

The two 2p electrons occupy separate orbitals with the same spin - not paired in one orbital.

Example: Nitrogen (1s² 2s² 2p³)

1s: [↑↓] 2s: [↑↓] 2p: [↑][↑][↑]

Figure 1.9: Electrons in Boxes for H through Ne

(Table showing electrons-in-boxes notation for elements H to Ne. Each row shows element symbol, configuration, and boxes for 1s, 2s, 2px, 2py, 2pz filled with up/down arrows. Highlight Hund's rule in C, N and spin-pair repulsion in O.)

Exam Tip

Spin-pair repulsion explains why the fourth electron in a p sub-shell must pair up with an existing electron - this costs energy, which is why there is a slight dip in ionisation energy between N and O in Period 2.

Shapes of s and p Orbitals

Figure 1.10: Shapes of s and p Orbitals

(Left: sphere labelled 's orbital' centred on nucleus. Right: three dumbbell shapes labelled pₓ, pᵧ, p_z oriented along their respective axes - all centred on the same nucleus and mutually perpendicular. Show the nucleus as a dot at the centre of each.)

Key Point

The shape of an orbital represents the region of space where there is a high probability of finding an electron (approximately 95% probability). Orbitals do not have sharp boundaries.

Free Radicals

Free Radical A species (atom, molecule or ion) that has one or more unpaired electrons. Free radicals are highly reactive.

Ionisation Energy

First Ionisation Energy (IE₁) The energy required to remove one mole of electrons from one mole of gaseous atoms of an element, to form one mole of gaseous ions with a single positive charge. Equation for First Ionisation Energy

X(g) → X⁺(g) + e⁻ ΔH = IE₁

State symbols are essential - ionisation energy is always defined for gaseous species.

Key Point

Ionisation energy is always endothermic (positive ΔH) - energy must be supplied to overcome the attraction between the nucleus and the electron.

Successive Ionisation Energies

Successive ionisation energies represent removing electrons one at a time from an increasingly positive ion:

Example: Aluminium

IE₁: Al(g) → Al⁺(g) + e⁻

IE₂: Al⁺(g) → Al²⁺(g) + e⁻

IE₃: Al²⁺(g) → Al³⁺(g) + e⁻

Factors Affecting Ionisation Energy

The ionisation energy of an element depends on the attraction between the nucleus and the outer electron. Four key factors influence this:

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