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v0.1.1436
NotesChemistryTopic 1.3Emission spectra and the electromagnetic spectrum
Back to Chemistry Topics
1.3.13 min read

Emission spectra and the electromagnetic spectrum

IB Chemistry • Unit 1

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Contents

  • Light, photons and the electromagnetic spectrum
  • Continuous vs line spectra
  • Evidence for discrete energy levels — and convergence
  • Exam-style question
The big idea: Light is part of the electromagnetic (EM) spectrum — a continuous range of waves from low-energy radio waves up to high-energy gamma rays, with visible light in the middle (red → violet).

Light travels in tiny packets of energy called photons. The key relationships are:

- higher frequency f → shorter wavelength λ → more energy per photon. - red light = low energy; violet/UV light = high energy.
Two given equations: The data booklet gives you both equations you need here:

- c = λf links wavelength and frequency (c is the fixed speed of light). - E = hf links a photon's frequency to its energy.

Put together: high frequency = short wavelength = high energy.

When you pass white light through a prism you get a continuous spectrum — an unbroken rainbow with every colour (wavelength) present. But when an element is heated or given electrical energy, it gives out a line spectrum — only a few specific coloured lines on a black background, at fixed wavelengths.

The visible hydrogen emission spectrum: a few coloured lines on black that get closer together (converge) toward the high-energy end — not a continuous rainbow.

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Continuous spectrum

  • An unbroken rainbow — all wavelengths present.
  • Produced by white light (e.g. a hot lamp filament).
  • Colours merge with no gaps.

Line (emission) spectrum

  • A few discrete bright lines on a black background.
  • Produced by an excited element (e.g. hydrogen gas).
  • Each element has its own unique pattern of lines.
Describing a line spectrum: If a question says describe the appearance of the hydrogen (or helium) emission spectrum, the marking point is: a series of discrete coloured lines (not a continuous rainbow) that get closer together (converge) toward the high-frequency / high-energy end.

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Why does hydrogen give only lines, not a full rainbow? Because the electron can only exist in fixed energy levels (it is quantised). When an excited electron falls from a higher level to a lower one, it emits a photon whose energy is exactly the gap between the two levels. A fixed set of gaps gives a fixed set of lines — that is the evidence that energy levels are discrete, not continuous.

Electrons sit in fixed energy levels. An excited electron falling back to a lower level emits a photon — the bigger the drop, the higher the photon energy.

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The size of the drop sets the photon's energy. Using the given equation, a bigger energy gap means a higher frequency line:

Planck's constant h is given in the data booklet (Section 2).
energy of one photon (J)
Planck's constant = 6.63 × 10⁻³⁴ J s
frequency of the light (Hz)
Why the lines converge: The energy levels themselves get closer together as you go up (toward the higher levels). So the transitions to a given level also get closer in energy, and the spectral lines converge (bunch up) toward the high-frequency / high-energy end. At the convergence limit, the electron has enough energy to leave the atom — this gives the ionisation energy.

Worked example — which line has more energy?

In the hydrogen spectrum, the red line has a wavelength of 656 nm and a violet line has 410 nm. Which line corresponds to the higher-energy photon, and why?

Solution

  1. Formula first — link wavelength to frequency:
  2. Shorter λ means higher f. The violet line (410 nm) has the shorter wavelength, so the higher frequency.
  3. Now link frequency to energy:
  4. Higher f → higher E, so the violet (410 nm) line is the higher-energy photon — it comes from a bigger electron drop.

Final answer

The 410 nm (violet) line — shorter λ → higher f → higher E (a larger energy-level gap).

How this is tested: S1.3.1 shows up as a quick Paper 1A MCQ ('what does the hydrogen line spectrum give evidence for?' or 'which transition emits the highest-energy radiation?') and a short Paper 2 outline/explain question.

The classic Paper 2 ask is to explain how the line spectrum supports discrete energy levels — for full marks you must link fixed lines → fixed energy gaps → quantised levels, and mention that the lines converge at high energy.
The highest-energy line: For 'which transition emits the highest-energy photon?', pick the biggest energy gap — that is an electron falling to n = 1 (the ground state) from the highest level. Lowest level, biggest drop, highest energy.

IB-style question — line spectrum as evidence (a)

When excited, hydrogen gas emits light that forms a line spectrum rather than a continuous spectrum. (a) Explain how this line spectrum provides evidence that the electron in a hydrogen atom occupies discrete energy levels. [2]

How to score the marks

  1. Mark 1 — fixed lines = fixed energy jumps. Each line is emitted when an electron falls from a higher level to a lower one, releasing a photon of a fixed energy (E = hf) equal to the gap between the levels.
  2. Mark 2 — only certain values are allowed. Because only specific wavelengths/lines appear (not a continuous range), only specific energy gaps are possible — so the energy levels must be discrete (quantised), not continuous.

Final answer

Each line corresponds to an electron dropping between two fixed levels, emitting a photon of fixed energy (E = hf). Only certain lines appear, so only certain energy gaps exist — the levels are discrete/quantised.

IB-style question — convergence and the highest-energy line (b)

(b) State and explain which electron transition in the hydrogen atom emits the highest-energy radiation, and state what happens to the spacing of the lines at higher frequency. [2]

How to score the marks

  1. Mark 1 — the transition. The transition with the largest energy gap emits the highest-energy photon: an electron falling to n = 1 (the ground state) from a very high level (the biggest possible drop).
  2. Mark 2 — the lines converge. At higher frequency/energy the lines get closer together (converge) because the energy levels themselves get closer together as n increases.

Final answer

Highest energy = electron falling to n = 1 (largest gap). The lines converge (get closer together) toward higher frequency.

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how the line emission spectrum of hydrogen provides evidence that the electron occupies discrete energy levels. [2] [2 marks]

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