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The size and color, at sometime, it will get too old and blow up, like a nova or supernova.

A young star is mostly hydrogen, undergoing nuclear fusion to form helium. As the star gets older, it has steadily more helium. Eventually, when it begins to run out of hydrogen, the helium will undergo fusion to form progressively heavier elements. By looking at the light from the star through a spectroscope, you can see markers that indicate the proportion of different elements, allowing you to estimate the star's age.

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