IB ChemistryStructure 33.13.1.6
3.1.6HL

Ionisation Energy Anomalies

Why Be→B and N→O break the periodic trend. Subshell energy and spin-pairing.

🟣 This is Higher Level (HL) content.

While first IE generally increases across Period 2, there are two anomalous dips that examiners love to test:

1st Ionisation Energy across Period 2

Ionisation Energy Period 2 0 500 1000 1500 2000 2500 Li Be B C N O F Ne Element (Period 2) 1st Ionisation Energy (kJ mol⁻¹) Be → B Dip N → O Dip

Anomaly 1: Be → B (Group 2 → 13)

Be: 1s² 2s². Electron removed from 2s subshell

B: 1s² 2s² 2p¹. Electron removed from 2p subshell

The 2p subshell is higher in energy than 2s (further from nucleus, less penetrating). Therefore the 2p electron in B is easier to remove despite higher Zeff.

Anomaly 2: N → O (Group 15 → 16)

N: 2p³. Three electrons each in separate p-orbitals (↑ ↑ ↑). No pairing

O: 2p⁴. One orbital now has a paired electron (↑↓ ↑ ↑)

The paired electron in O experiences spin-pairing repulsion within the same orbital. This raises its energy and makes it easier to remove, so O has a lower IE than expected.

⚠️ Examiner Trap

The same anomalies repeat in Period 3: Mg→Al (s→p subshell) and P→S (spin-pairing). You must be able to explain both using orbital diagrams.

← 3.1.5 Transition ElementsS3.1.7 IE Discontinuities →