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Scientists call a star that is fusing hydrogen to helium in its core a main sequence star. Main sequence stars make up around 90% of the universe's stellar population. They range in luminosity, color, and size - from a tenth to 200 times the Sun's mass - and live for millions to billions of years. For Stargazers: Many main sequence.. However, the brightness of a star depends on its composition and how far it is from the planet. Astronomers define star brightness in terms of apparent magnitude — how bright the star appears.