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v0.1.1040
NotesPhysicsTopic 5.1Energy levels and atomic spectra
Back to Physics Topics
5.1.22 min read

Energy levels and atomic spectra

IB Physics • Unit 5

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Contents

  • Energy levels and line spectra
  • Photon energy: E = hf = hc/λ
  • Exam-style question
The big idea: An atom can only hold a few allowed energies — never the values in between. These are its energy levels (we say the energy is quantised: it comes in fixed steps).

When an electron drops from a higher level to a lower one, the energy it loses leaves as a single packet of light — a photon.

Because only certain drops are allowed, an atom gives out only certain colours — a pattern of separate lines called a line spectrum.

[Diagram: phys-energy-levels] - Available in full study mode

New words, plainly: Quantised = only fixed values are allowed (like stairs, not a ramp).

Photon = one tiny packet of light energy.

Transition = an electron jumping between two levels.

Line spectrum = the set of separate lines (colours) an atom gives out or takes in.

Emission spectrum

  • Electron drops to a lower level and gives out a photon
  • You see bright coloured lines on a dark background
  • Each line = one allowed energy gap in the atom

Absorption spectrum

  • Electron absorbs a photon and jumps up to a higher level
  • You see dark lines missing from a continuous rainbow
  • The same gaps are missing as the emission lines — same atom, same energies
Why a line spectrum is a fingerprint: Every element has its own set of energy levels, so it has its own pattern of lines.

That is how we match a spectrum to an element — and how we know which energy-level diagram a spectrum came from.

The energy a photon carries equals the gap between the two levels. The data booklet gives two ways to link that energy to the light:

Photon energy from frequency (given in the data booklet). E in joules, h is the Planck constant, f in hertz.
energy of the photon — equals the energy lost in the jump (J)
Planck constant, 6.63 × 10⁻³⁴ J s (given)
frequency of the emitted (or absorbed) light (Hz)
Photon energy from wavelength (given). Use this when the question gives or asks for a wavelength λ. Bigger E → shorter λ.
energy of the photon — equals the energy of the jump (J)
Planck constant, 6.63 × 10⁻³⁴ J s (given)
speed of light, 3.00 × 10⁸ m s⁻¹ (given)
wavelength of the light (m)
Bigger drop → shorter wavelength: From , a bigger energy gap means a bigger E, which means a shorter wavelength λ (and higher frequency).

So the biggest drop makes the shortest-wavelength line; the smallest drop makes the longest-wavelength line.

[Diagram: phys-energy-levels] - Available in full study mode

Worked example — wavelength of an emitted photon

An electron in an atom drops between two levels and loses 3.0 × 10⁻¹⁹ J of energy. Find the wavelength of the photon it emits. (h = 6.63 × 10⁻³⁴ J s, c = 3.00 × 10⁸ m s⁻¹.)

Solution

  1. The photon energy equals the energy lost in the jump, so start from the given wavelength formula:
  2. Rearrange to make the wavelength λ the subject:
  3. Put in the numbers (h = 6.63 × 10⁻³⁴, c = 3.00 × 10⁸, E = 3.0 × 10⁻¹⁹):
  4. Work it out — keep the unit:

Final answer

λ ≈ 6.6 × 10⁻⁷ m (about 660 nm — red light). A small energy gap gives a long wavelength.

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How this is tested: Energy levels and spectra are almost always a Paper 1A multiple-choice question.

- Paper 1A — match: match an emission-line pattern to the correct set of energy levels (more gaps → more lines). - Paper 1A — longest wavelength: pick the transition that emits the longest-wavelength photon — that is the smallest energy drop. - Paper 1A — count the lines: given an electron falling from level n to the ground state, find how many different wavelengths are possible. - Paper 2: use or to turn a level gap into a frequency or wavelength.

Classic trap: thinking the biggest drop gives the longest wavelength — it's the opposite (biggest drop = shortest λ).
Counting distinct wavelengths: Each different gap between two levels makes one line. From level n down to the ground state, the number of different downward jumps is n(n − 1) ÷ 2.

For n = 3 that is 3 lines (3→1, 3→2, 2→1); for n = 4 it is 6 lines.

[Diagram: phys-energy-levels] - Available in full study mode

IB-style question — (a) how many emission wavelengths

In a particular atom an electron is excited to the third level (n = 3). As the atoms in a sample relax, the electrons fall back to the ground state by every possible route. How many different wavelengths can appear in the emission spectrum?

Solution

  1. Each distinct downward jump between two levels gives one wavelength. List the jumps possible from n = 3:
  2. From n = 3: the jumps are 3→2, 3→1 and 2→1 — three different gaps.
  3. Three different energy gaps → three different photon energies → three different wavelengths.

Final answer

3 different wavelengths (3→2, 3→1 and 2→1). The shortcut n(n − 1)/2 = 3(2)/2 = 3 agrees.

IB-style question — (b) the longest-wavelength line

Using the same three levels, state which transition produces the photon with the LONGEST wavelength, and explain why.

Solution

  1. Longest wavelength means the smallest photon energy, because — small E ↔ large λ.
  2. The smallest energy drop is the jump between the two closest levels: 3→2.
  3. So the 3→2 jump loses the least energy and makes the longest-wavelength photon.

Final answer

The 3→2 transition (the smallest energy gap) gives the longest-wavelength photon, because a smaller energy means a larger wavelength.

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why the energy of an electron in an atom can only take certain values rather than any value at all. [1 mark]

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5.1.1Nuclear model and atomic structure
5.1.3The electronvolt
5.1.4Quantisation of charge
5.3.1Types of radiation and their properties
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