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AP® Chemistry · Unit 3 · Topic 3.12

Properties of Photons: Revision Notes (Chemistry 3.12)

One-page recap of photon energy, c = λν and E = hν, energy per mole of photons and energy-level diagrams, with the unit slips that cost marks.

Short on time? This page is the recap. For explanations, a diagram and worked examples, use the full study guide.

Recap

  • Light comes in photons. Each photon’s energy depends only on its frequency.
  • Absorbing a photon raises the energy of an atom or molecule by exactly the photon’s energy. Emitting a photon lowers it by exactly that amount.
  • Photon energy = difference between two levels: E(photon) = E(upper) − E(lower).
  • Only photons whose energy matches a gap are absorbed or emitted, so spectra show sharp lines.
  • Brightness = number of photons. It does not change the energy of each photon.

Key relationships

Relationship Symbols and units Use it to
c = λν c = 2.998 × 10⁸ m s⁻¹; λ in m; ν in s⁻¹ (Hz) convert between wavelength and frequency
E = hν E in J per photon; h = 6.626 × 10⁻³⁴ J s find the energy of one photon from its frequency
E = hc/λ λ in m go straight from wavelength to energy
E(per mol) = E(per photon) × N_A N_A = 6.022 × 10²³ mol⁻¹; ÷ 1000 for kJ compare with bond energies in kJ mol⁻¹

Proportions: λ and ν are inversely proportional; E and ν are directly proportional; E and λ are inversely proportional.

Assumptions behind the numbers

  • The light travels at c, its speed in a vacuum (air changes it by less than 0.1%, too little to matter here).
  • Each absorption or emission involves one photon and one atom or molecule.
  • The energy levels are fixed values, so each gap gives one sharp wavelength.

Mistakes to avoid

  1. Not converting nm to m. 1 nm = 10⁻⁹ m. Do it first.
  2. Per photon vs per mole. E = hν is per photon; multiply by N_A for per mole.
  3. Forgetting J → kJ. Divide by 1000 at the end.
  4. Using the level energy instead of the gap. Always subtract: upper − lower.
  5. Negative photon energy. If you get one, you subtracted the wrong way round.
  6. Thinking brighter light can reach a bigger gap. One photon, one transition: energy per photon decides.

Quick self-check

  1. What is the frequency of light with λ = 5.00 × 10⁻⁷ m? (6.00 × 10¹⁴ s⁻¹)
  2. What is the energy of one photon of frequency 1.00 × 10¹⁵ s⁻¹? (6.63 × 10⁻¹⁹ J)
  3. An atom drops from a level at −3.0 × 10⁻¹⁹ J to one at −7.0 × 10⁻¹⁹ J. What is the energy of the emitted photon? (4.0 × 10⁻¹⁹ J)

Next: practice questions.

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