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AP® Physics 2: Algebra-Based · Unit 15 · Topic 15.3

Emission and Absorption Spectra: Topic Checklist (Physics 2 15.3)

Specific “I can…” statements for emission and absorption spectra, each linked to the guide section and practice question that shows whether you can really do it.

Work through the list without notes. If you cannot do a statement, follow its link, then come back. Guide = study guide; Practice = practice questions.

Understanding

  • I can explain that the atom is a system of an electron and a nucleus, and that a change of state is a change in their interaction energy. (Guide: “The atom as a system”)
  • I can explain why bound energy levels are negative and what the ground state, excited states and ionization mean. (Guide: “The atom as a system”; Practice Q4)
  • I can state that a photon is absorbed or emitted only when its energy equals the gap between two states, and explain why this gives single wavelengths. (Guide: “Photons in, photons out”; Practice Q1)
  • I can describe how emission and absorption spectra form, and why a cool gas shows fewer absorption lines than the hot gas emits. (Guide: Figure 2; Practice Q2, Q6c)

Calculation and skills

  • I can read an energy level diagram and find the energy, wavelength and frequency of the photon for any transition. (Guide: Worked example 1; Practice Q3, Q5)
  • I can count and list all the possible emission lines from a given level. (Practice Q5a)
  • I can decide whether a photon of given energy is absorbed by an atom in a given state. (Guide: Worked example 2; Practice Q1, Q7d)
  • I can find the binding energy from any level and the kinetic energy of an electron freed by a photon. (Guide: “Binding energy and ionization”; Practice Q4, Q7d)
  • I can build an energy level diagram from measured line wavelengths. (Practice Q7)

Reasoning

  • I can use emission or absorption lines, compared with reference spectra, to decide which elements are present, and say why one matching line is not enough. (Guide: “Line spectra and what they tell you”; Practice Q6)
  • I can explain why absorption lines look dark even though the atoms re-emit. (Practice Q2, Q6d)
  • I can justify which transition produced a line using energy conservation. (Practice Q7c)

All ticked? Move on to Topic 15.4, Blackbody Radiation, or return to the course roadmap.

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