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Every star has its own life cycle, ranging from a few million to trillions. Main sequence stars make up around 90% of the universe’s stellar population Of the tens of billions of trillions of stars in.

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[1] the nearest star to earth is the sun Scientists call a star that is fusing hydrogen to helium in its core a main sequence star Many other stars are visible to the naked eye at night

And what happens when they die

These star facts explain the science of the night sky. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star’s interior and then radiates into outer space. Stars are huge celestial bodies made mostly of hydrogen and helium that produce light and heat from the churning nuclear forges inside their cores.