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PH23-01 Physics Coming soon

How a star forms and why it is stable (triple)

PH23-01

This lesson is coming soon.

In this lesson

Details to come.

For: AQA GCSE 8463, Edexcel GCSE 1PH0, OCR GCSE J249

On the specification

BoardSpecStatement
AQA GCSE 84634.8.1.1Our solar system
Edexcel GCSE 1PH07.16PDescribe the evolution of stars of similar mass to the Sun through the following stages: a nebula b star (main sequence) c red giant d white dwarf
Edexcel GCSE 1PH07.17PExplain how the balance between thermal expansion and gravity affects the life cycle of stars
Edexcel GCSE 1PH07.18PDescribe the evolution of stars with a mass larger than the Sun
OCR GCSE J249P8.3cRecall that our Sun was formed from dust and gas drawn together by gravity and explain how this caused fusion reactions, leading to equilibrium between gravitational collapse and expansion due to the energy released during fusion
For teachers

This GCSE Physics lesson teaches how a star forms and why it is stable (triple). It suits Foundation and Higher tier students.