By conducting experimental research with matter 10 million times denser and 25 times denser than that found at the centre of the sun, researchers have determined the nature of the nuclear processes that occur within intermediate-mass stars. Our understanding of the deaths of both low and high mass stars are fairly sound, but the team’s findings could change how we think about the fate of stars that lie in between. They suggest that such stars may not collapse, as previously believed, but instead end their lives in a spectacular explosion. How a star evolves is very much dictated by its…
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