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The Periodic Table

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Edexcel IAL Chemistry · Topic 1.5

The Periodic Table

Big idea: as you move across a period, atoms get harder to ionise but easier to bond tightly in a metal lattice — and both trends come down to one thing: how strongly the nucleus pulls on the outer electrons.

Summary — the whole chapter in one scan

  • First ionisation energy generally increases across a period (left → right) because nuclear charge goes up while shielding stays about the same, so the atom shrinks and holds its electrons tighter.
  • First ionisation energy decreases down a group because extra electron shells add distance and shielding, which outweighs the bigger nuclear charge.
  • There are two predictable "dips" in the ionisation energy graph across Period 2 and Period 3 — one from a change in subshell (Be→B, Mg→Al) and one from electron-electron spin-pair repulsion (N→O, P→S).
  • Melting points across Period 3 rise steeply from Na to Si, then crash from Si to Ar — because the bonding and structure change completely partway through the period.
  • Na, Mg, Al are giant metallic structures; Si is a giant covalent (molecular) structure; P, S, Cl, Ar are simple molecular structures held together by weak intermolecular forces.

1. Ionisation Energy Across a Period

First, let's be precise about what "first ionisation energy" (IE₁) actually means, because half of getting this topic right is knowing the definition cold:

Definition First ionisation energy is the energy required to remove one electron from each atom in one mole of gaseous atoms, to form one mole of gaseous 1+ ions.

X(g) → X⁺(g) + e⁻

The periodic table isn't just a random grid — elements are lined up in order of increasing atomic number, arranged into groups (columns) and periods (rows). Because electron configuration repeats in a pattern as atomic number increases, properties like ionisation energy repeat too. That repeating pattern is called periodicity — and it's the reason a graph of IE₁ against atomic number looks like a jagged sawtooth that resets at the start of every new period.

FIRST IONISATION ENERGY (kJ/mol) — Period 2 example 2500 | He | * 2000 | | 1500 | N F Ne | * \ * * 1200 | C * O | * \ / 900 | Be * | * \ / 600 | / B | / * 300 | H Li | * * 0 +--------------------------------------------- Na 1 2 3 4 5 6 7 8 9 10 11 (atomic number) Notice: overall trend rises across the period, but dips at Be→B and N→O. Then it CRASHES back down at Na — a new period, a new outer shell, much easier to remove an electron.

Think of it like this: imagine the nucleus is a magnet and the outer electrons are paperclips stuck to it. As you move across a period, you're adding protons to the nucleus (stronger magnet) but the paperclips are still in the same shell — same rough distance away. A stronger magnet pulling on paperclips at the same distance means it's harder to pull one off. That's the whole trend in one sentence.

Why ionisation energy increases across a period

Four linked facts, each one causing the next:

  1. Nuclear charge increases
  2. Shielding stays roughly constant
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Also in the full note
  • 2. Ionisation Energy Down a Group
  • 3. Thermal Trends — Melting Points Across Period 3
  • What to Memorise
  • Concepts Checklist
  • Exam Tips & Common Mistakes
  • The two dips in Period 2 (and why they matter)
  • Dip 1 — Beryllium → Boron (subshell change)
  • Dip 2 — Nitrogen → Oxygen (spin-pair repulsion)
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