The Sun didn’t emerge from a single, smooth collapse. Instead, the vast solar nebula fragmented into multiple dense clumps due to Jeans instability—where gravity overcomes gas pressure, causing different regions to collapse at varying rates. This chaotic process set the stage for the formation of our star and the planets that orbit it today. But why did the Sun become the dominant object in our solar system? And what forces shaped its fiery birth? Let’s unravel the origins of the star that gives us life!
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