Researchers from Michigan State
University are using Mira to perform large-scale 3D simulations of the final
moments of a supernova's life cycle. While the 3D simulation approach is still
in its infancy, early results indicate that the models are providing a clearer
picture than ever before of the mechanisms that drive supernova explosions.
At the end of their life cycles,
these massive stars explode in spectacular fashion, scattering their guts (which
consist of carbon, iron and basically all other natural elements) across the
cosmos. These elements go on to form new stars, solar systems and everything
else in the universe, including the building blocks for life on Earth.
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