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Sagot :
A star's mass is the most critical factor determining what happens in every phase of its life.
A star's life still up in the air by its mass. The bigger its mass, the shorter its life cycle. A star's still up in the air by how much matter that is accessible in its cloud, the goliath haze of gas and dust from which it was conceived. After some time, the hydrogen gas in the cloud is arranged by gravity and it begins to spin. As the gas spins faster, it heats up and becomes as a protostar. At last the temperature reaches 15,000,000 degrees and atomic fusion occurs in the cloud's center. The cloud begins to gleam brilliantly, contracts a bit, and becomes stable. It is presently a fundamental sequence star and will stay in this stage, shining for millions to billions of years to come. This is the stage our Sun is at the present moment.
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