Energy levels in atoms and line spectra

Physics A2 · Quantum physics. The idea in plain words, the rules to remember, the mistake to avoid and a worked example, written and checked by Mega Lecture.

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The idea

An electron in an isolated atom can have only certain fixed energies, called discrete energy levels. It cannot have an energy between two levels. The levels are given negative values because a free electron at rest is taken to have zero energy, and a bound electron has less than that.

When an electron falls to a lower level it emits one photon. The photon energy equals the difference between the two levels. Only certain differences exist, so only certain wavelengths are emitted. This gives an emission line spectrum: bright lines on a dark background.

A cool gas absorbs photons whose energy exactly matches a jump upwards. White light passed through it shows dark lines, an absorption line spectrum.

Rules to remember

Common mistake

Students use the energy of one level as the photon energy. The photon energy is the difference between two levels, and it must be changed from eV to joules before using hf or hc/λ.

Worked example

An electron in an atom falls from a level of −1.6 eV to a level of −4.1 eV. What is the wavelength of the photon emitted?

  1. Energy difference = (−1.6) − (−4.1) = 2.5 eV.
  2. In joules: 2.5 × 1.60 × 10−19 = 4.0 × 10−19 J.
  3. λ = hc/E = (6.63 × 10−34 × 3.00 × 108) ÷ (4.0 × 10−19) = 4.97 × 10−7 m.

Answer: About 5.0 × 10−7 m (500 nm).

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