Galaxy Classification
Students drag galaxies into the correct Hubble classification zone using visible structural clues, then use the feedback to connect galaxy morphology with stellar…
Home › Interactives › Earth & Space Sciences › Nuclear Fusion Core Simulator
Earth & Space Sciences · Stars & the Universe
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.
Change one variable at a time and ask students to predict the direction of change in energy output.
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Students drag galaxies into the correct Hubble classification zone using visible structural clues, then use the feedback to connect galaxy morphology with stellar…
Students compare three-dimensional representations of the major galaxy types and inspect how shape, stellar population, gas content and star-formation behaviour…
Students explore a star alongside its position on a Hertzsprung–Russell diagram, changing stellar mass and relating temperature, luminosity, radius and evolutionary…
Students alter stellar parameters such as core temperature, fusion support and opacity and observe whether inward gravity and outward pressure remain balanced. It shows…
Students move a galaxy through cosmological distance, compare rest and observed spectral lines, calculate redshift from the wavelength shift and connect recession…
Students explore the layered structure of the Sun and compare the physical conditions and roles of the core, radiative zone, convective zone, photosphere, chromosphere…
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.