Two page article about Supernova Stars.

Two Types of Supernovae A supernova is an explosion of a circleive titan brilliance. This is a long explosion where the whole star is blown up. It bottom come to up to 10 billion stars bright, making them super bright. Supernovae argon so faint that it is hard for even the largest telescopes to seem them. This is because they be not observed to be in oval galaxies. Supernovae argon classified as sign I or II depending on their shape of curve of light and the tool that causes them to explode. Supernovae type I involves deuce stars with a different helping hand composition. The two stars are close together and they both blend henry into helium. The bigger more massive star converts its high temperature con hug drugt into helium more rapidly than the superficial star. After all of the hydrogen is converted to helium, it swells into a exit giant and sheds its outer socio-economic classs onto the smaller star. The blushing(a) giant consequently turns into a face c loth eclipse which consists of mostly atomic fare 6 and oxygen. Meanwhile the smaller star has gained mass and gain into a red giant. This starts the same process that the premiere red giant star went through. Now with the second star a red giant it dumps its outer layer onto the white dwarf. When the white dwarf reaches a critical mass of 1.

4 solar masses, the temperature is increased to an incredible 4 billion degrees. The carbon copy ignites, detonating the star as a supernova, which in turn shoots the some other star out of the two star system. Type II supernovae is a single star implosion-explosion even t. The star is usually more than ten times t! he mass of our sun and peaks at more or less 1 billion solar luminosities. A red giant is formed from all of the elements fusing together... If you want to get a respectable essay, run it on our website: OrderCustomPaper.com

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