#HIGHLIGHT_SUMMARY-1049Highlight Correct SummaryCore & AcademicMedium
Question 50
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When we look at the periodic table, it is fascinating to trace the origins of the atoms that make up our world. The early universe, moments after the Big Bang, consisted almost entirely of hydrogen and helium, the simplest elements. There was practically nothing else. So, where did the carbon in our cells, the calcium in our bones, or the iron in our blood come from? The answer lies in the fiery cores of stars. For billions of years, stars function as cosmic factories, fusing simple atoms into heavier ones through nuclear fusion. However, ordinary stellar fusion can generally only create elements up to iron. To generate anything heavier, or to disperse these materials into space where they can coalesce into rocky planets and living organisms, a cataclysmic event is required: a supernova. When a massive star collapses and explodes, it not only creates heavier elements like gold and uranium but also blasts this enriched debris across the galaxy. Essentially, the violent death of stars is a prerequisite for biological existence; we are, in a very real sense, made of stardust.
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