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A star will use fusion to combine lighter atoms into heavier atoms. A main-sequence star (that's the majority of stars) will convert hydrogen-1 into helium-4, so in this case, hydrogen-1 is the fuel. Once it starts running out of hydrogen-1, it will start fusing the helium into heavier elements - in which case the main fuel will be the helium-4. Later in the life cycle of a star, the fuel can be even heavier elements.

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6y ago
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6y ago

Mostly hydrogen. Later on, helium and finally heavier elements.

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Q: What Fuel does a Star burn to create its own energy?
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