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The life expectancy of a star (E) depends on its mass (M), roughly following the model of E = M-2.5.

For a star with a mass twice that of our sun (enter 2 in place of `M`), then the lifespan will give 0.177. Our suns lifespan is around 10 billion years, so this would equate to 1.77 billion years.

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Q: If a star is twice as massive as the sun how will its lifespan compare?
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