Thursday, October 27, 2011

Stellar Nuclear Fusion

Hydrogen (75% of the Sun) furnishes nuclear fule for stars like the Sun. Because the core of a typical star is so violent and hot, hydrogen nuclei are separated from their electrons. in the star's core, the great pressure of overlying material forces the protons to collide so violently that the nuclei fuse together. The nuclear reactions fuse the nuclei of four hydrogen atoms into a single helium nucleus, liberating energy in the process and producing a star's light and heat. In this fashion, more than 4 million tons of the Sun's mass are converted into energy every second.

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