The Life Cycle of Stars

Paper Summary:

In order to shed some light onthe processes involved in the stars' life cycle, this paper discusses and analyzes how, throughout its 'life,' a star will remain dependent on other stars for its eventual re-birth--that is, the creation of another kind of a star. In line with the main topic of this paper, the discussion and analysis argue that the life cycle of a star is an interdependent and recurring process, mainly because stars depend on other stars to re-generate or create another star.

From the Paper:

"The second phase, the star's death, occurs when the star has finally used up its hydrogen atoms, and can no longer generate energy from its stellar body. As this happens, the star is "pulled" by the gravity and will burn its helium to become carbon, becoming a red giant. The dying star will be pulled towards the gravity because it will no longer have the counterforce that it once had (force from the energy radiated from it) in order to balance the two forces (gravity and energy pressure). Once helium gases were burned out or exhausted from the stellar body, carbon will be produced and scattered. The dead star will eventually have a carbon core, cool down, and become a white dwarf."

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