Learning objective
Use Wien's law to estimate surface temperature.
Read the explanation, check the common trap, then practise with flashcards and questions.
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Topic
Classification of stars
Subtopic
Temperature and black-body radiation
Aqa A Level PhysicsAstrophysics
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Quick explanation
Use Wien's law to estimate surface temperature
- This point belongs to Classification of stars, especially Temperature and black-body radiation.
- You need to be able to use Wien's law to estimate surface temperature.
- The key ideas to know are surface temperature and Wien's law.
- Use the linked flashcards and practice questions to check recall, then practise applying the idea in an exam-style answer.
Key concepts
surface temperatureWien's law
Why it matters
This objective helps connect Temperature and black-body radiation to exam-style questions, flashcards, and revision notes for Classification of stars.
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Revision notestopic notes
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Open revision notesRelated learning objectives
- Define luminosity as power output of a star.
Classification by luminosity
- Use inverse-square relationships for apparent brightness.
Classification by luminosity
- Compare apparent brightness and luminosity.
Classification by luminosity
- Interpret brightness data for stars.
Classification by luminosity
- Distinguish apparent magnitude from absolute magnitude.
Absolute magnitude