Salam Academy
Paper 1 · Module

Atomic structure

2 subtopics≈ 85 min in total
  1. Particles, isotopes and orbitals

    Electrons occupy shells (n=1,2,3…n=1,2,3…) divided into subshells (s, p, d), each made of orbitals holding at most two electrons of opposite spin. Subshells fill in order of energy: 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p. Exceptions: Cr is [Ar] 3d⁵ 4s¹ and Cu is [Ar] 3d¹⁰ 4s¹. Transition-metal ions lose 4s electrons first. Relative atomic mass is the weighted mean from a mass spectrum: Ar=∑(m/z×abundance)∑abundanceA_r=\frac{\sum(m/z\times\text{abundance})}{\sum\text{abundance}}.

    ≈ 45 min
  2. Ionisation energies

    The first ionisation energy is the energy needed to remove one mole of electrons from one mole of gaseous atoms: X(g)→X+(g)+e−\mathrm{X(g)\rightarrow X^+(g)+e^-}. It depends on nuclear charge, distance of the outer electron from the nucleus and shielding. Across a period it generally increases (more protons, similar shielding); down a group it decreases (further away, more shielding). Dips occur at Group 13 (new p subshell, higher energy) and Group 16 (spin-pair repulsion). Successive ionisation energies show big jumps when an inner shell is broken into.

    ≈ 40 min