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Earth & Space Sciences · Stars & the Universe

Nuclear Fusion Core Simulator, Years 11–12

Students vary stellar-core temperature, density and hydrogen content and observe changes in proton–proton fusion rate, energy output and pressure support. The full interactive is available to licensed Education Universe users.

Years 11–12, UndergraduateExplorer

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Learning outcomes

Teaching guidance

Change one variable at a time and ask students to predict the direction of change in energy output.

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Start a free 30-day trial with class codes and progress tracking, or talk to us about your school's licence.

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Nuclear Fusion Core Simulator is one of the licensed interactives in The Education Universe. This page describes it; teachers use it in lessons and classes with a licence or the free trial.