| Lesson Plan | |
| Grade: | Date: 17/01/2026 |
| Subject: Physics | |
| Lesson Topic: recall and use hf = E1 – E2 | |
Learning Objective/s:
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Materials Needed:
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Introduction: Begin with a striking image of the red H‑α nebular line to spark curiosity. Review the idea that electrons occupy discrete energy levels and that transitions produce photons. State that today students will master the formula hf = E1 – E2 and will be able to predict wavelengths of atomic spectra. |
Lesson Structure:
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Conclusion: Summarise how the hf = E1 – E2 relationship links energy differences to observable spectral lines. Collect exit tickets to gauge understanding, and assign homework: three additional transition problems (including one from the Lyman series) to reinforce conversion skills. |
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