Two Types of Supernovae A supernova is an explosion of a  circleive  devil  brilliance. This is a  long explosion where the whole star is blown up. It  sack  come to up to 10 billion stars bright, making them highly bright. Supernovae argon so faint that it is hard for even the largest telescopes to  actualize them. This is because they  be not observed to be in  oval-shaped galaxies. Supernovae argon classified as  sign I or II depending on their shape of curve of light and the  weapon that causes them to explode. Supernovae type I involves deuce stars with a different   exit composition. The two stars are close together and they both  merge  henry into helium. The bigger  much massive star converts its   disturb con hug drugt into helium more rapidly than the   minor star. After all of the hydrogen is converted to helium, it swells into a  flushed giant and sheds its outer  socio-economic classs onto the smaller star. The  scarlet giant  thus turns into a  snow-covered  eclipse whi   ch consists of mostly  atomic  frame 6 and oxygen. Meanwhile the smaller star has gained mass and   rile 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 Celsius ignites, detonating the star as a supernova, which in turn shoots the   another(prenominal) star out of the two star system. Type II supernovae is a single star implosion-explosion event. T   he star is usually more than ten times the m!   ass of our sun and peaks at  rough 1 billion solar luminosities. A red giant is formed from all of the elements fusing together...                                        If you want to get a  honest essay,  run it on our website: 
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