The Sun

Like other wizards, the Sun shines by fusing total warming into helium in its subject matter. Without the power that this conversion fulfill generates, a atomic number 82 would give out under its bear immense weight. The heavier the star is, the fast it consumes its total heat and the instead it dies. By the time our Sun becomes a old citizen, just about of its hydrogen bequeath be gone and its karyon will consist of pure helium. With no more hydrogen left at the core, the nuclear reactions that occurred there die out. And helium cannot tan at the low temperatures associated with hydrogen fusion. Without the outward wring of lance of light from the nuclear reactions, the core of the Sun will jut to shrink. With the inward crush of matter, the remaining hydrogen around the core heats up enough to begin a new vomit of fusion. The radiation produced slowly pushes the outer layers of the Sun out at one time more. As the Sun now reaches a critical temperature, he lium atoms start to fuse together to digit carbon. This reaction halts the get around of the core, but not for long. atomic number 2 burns much faster than hydrogen. The intense heat expels a massive wave of radiation that pushes the Suns atmosphere out further.

on the button over 7 one million million million years from now, the Sun will transform itself into a sibyllic red giant, 100 times its present size and possibly 2,000 times a luminous. As it continues to expand, its gas thins and clears. Light from the baggy core shines through outer layers of gas for the first time. The star is now pulsating from fusion reactions in a helium point out around a carbon core, driving th e Suns outermost layers even farther out in! to space. They eventually form a desirous sphere called a planetary nebula. The Suns now carbonized core shrinks... If you extremity to get a full essay, order it on our website: OrderEssay.net

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