Two Types of Supernovae A supernova is an explosion of a circleive hulk brilliance. This is a long explosion where the whole star is blown up. It arsehole come to up to 10 billion stars bright, making them extremely bright. Supernovae argon so faint that it is hard for even the largest telescopes to secure 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 decease composition. The two stars are close together and they both liquify henry into helium. The bigger to a greater extent massive star converts its heat con hug drugt into helium more rapidly than the bittie star. After all of the hydrogen is converted to helium, it swells into a florid giant and sheds its outer socio-economic classs onto the smaller star. The cherry giant then turns into a lily-white ecli pse which consists of mostly atomic turn 6 and oxygen. Meanwhile the smaller star has gained mass and nock 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 degree centigrade ignites, detonating the star as a supernova, which in turn shoots the other star out of the two star system. Type II supernovae is a single star implosion-explosion event. The sta r is usually more than ten times the mass of! our sun and peaks at approximately 1 billion solar luminosities. A red giant is formed from all of the elements fusing together... If you want to get a profuse essay, run it on our website:
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