Why atoms give line spectra, how electrons are arranged in energy levels and orbitals, and how to write any configuration.
This is the Standard Level lesson, covering S1.3.1–S1.3.5. Taking Chemistry at Higher Level? The HL version adds ionisation energy (S1.3.6–S1.3.7) — using the hydrogen spectrum's convergence and successive ionisation energies as evidence for the levels.
When electrons are excited to higher energy levels and then fall back down, they emit photons of specific energies — giving a line spectrum, not a continuous rainbow. The fixed lines are direct evidence that electrons occupy discrete energy levels. The lines converge (get closer) at higher energy. Click a jump down to level n=2 (the visible Balmer lines):
Each main energy level n holds up to 2n² electrons (n=1 → 2; n=2 → 8; n=3 → 18). Each level is divided into sub-levels — s, p, d, f — of rising energy, made of orbitals. Each orbital holds 2 electrons of opposite spin. An s sub-level has 1 orbital (2 e⁻), p has 3 (6 e⁻), d has 5 (10 e⁻).
Electrons fill from lowest energy up (Aufbau), one per orbital before pairing (Hund), with opposite spins (Pauli). Drag the slider to change the atomic number and watch the orbitals fill:
Two exceptions you must know: chromium (Cr, Z=24) is [Ar]3d⁵4s¹ and copper (Cu, Z=29) is [Ar]3d¹⁰4s¹ — a half-full or full d sub-level is extra stable, so one 4s electron shifts into 3d.
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