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The mass of a star significantly influences its lifespan on the Hertzsprung-Russell diagram, with more massive stars burning through their nuclear fuel much more quickly than less massive ones. High-mass stars (e.g., those greater than 8 solar masses) have shorter lifespans, often only a few million years, as they rapidly fuse hydrogen into heavier elements. In contrast, low-mass stars (like red dwarfs) can remain on the main sequence for billions of years, slowly converting hydrogen into helium. Consequently, the star's position on the diagram and its evolutionary path are closely linked to its mass.

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4d ago

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