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.