Objectives

Lesson outcomes

  • Use Wien's displacement law to estimate the surface temperature of a star from its spectrum.
  • Use the Stefan-Boltzmann law to relate a star's luminosity, radius, and surface temperature.
  • Combine Wien's displacement law and the Stefan-Boltzmann law to estimate the radius of a star.
Syllabus

CIE 9702 syllabus points

3 linked

Lesson Notes

Teacher and student guidance

Overview

Use standard candles to estimate astronomical distances.

Key knowledge and explanations

  • Main idea: Use standard candles to estimate astronomical distances.
  • Key definitions, models, equations, or diagrams to introduce.
  • One worked example, demonstration, or observation that makes the idea concrete.

Lesson flow

  1. Start with prior knowledge, context, or a short recall task.
  2. Work through the main explanation, method, diagram, or calculation for this lesson.
  3. Complete guided practice, discussion, calculations, or practical application.
  4. Review the learning with an exit prompt, short question, or summary task.

Checks for understanding

  • Use a hinge question aligned to the main objective(s) to check your understanding.
  • Use a short verbal, written, or numerical response to check for secure understanding.

Common mistakes or misconceptions

  • Watch for the likely misconception, error, or weak step in this lesson.
  • Review the comparison, model answer, or explanation that will correct it.

Follow-up

  • Complete the homework, retrieval task, or resource revisit linked to this lesson.
  • Note what you need to carry forward into the next lesson.
Lesson Resources

Materials for this lesson

Embed videos, slide decks, documents, or direct links in the frontmatter for each lesson.

Worksheet

Stefan-Boltzmann Law - Practice Questions

Stefan-Boltzmann Law - Practice Questions

Open resource
Worksheet

Wien’s Law Practice Questions

Wien’s Law Practice Questions

Open resource