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An immense collection of very light elements. A star is over 95% hydrogen with trace amounts of helium, oxygen, carbon, and other heavy elements. The star derives its energy from a thermonuclear reaction initieted by the pressure created by the [gravitational pull] of the gasses inward. A star will burn for millions if not billions of years before the hydrogen supply is depleted and the star's [nuclear fusion] reaction fails. The star will then explode and remove an outer layer of gasses and then collapse into a dense state. Average stars collapse into Dwarf Stars while massive ones form neutro stars of [black holes].
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