Blue supergiant stars are staller evolutions that have resulted over millions of years. Stars during the main sequence phase spend a majority of their lives. During the main sequence stage, the star converts hydrogen to helium by nuclear fusion in the cores of stars the process also known as proton-proton chain. After spending of hydrogen fuel, the star will collapse and heat up rapidly causing the outer layers to expand inwards. When the core is very hot, the energy spreads through the interior of the star’s large surface area. The different fusion rates of different elements vary wildly to ...
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