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Ask Ethan: When do stars flip essentially the most mass into power? | by Ethan Siegel | Begins With A Bang! | Might, 2025

swissnewshub by swissnewshub
2 May 2025
Reading Time: 4 mins read
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Ask Ethan: When do stars flip essentially the most mass into power? | by Ethan Siegel | Begins With A Bang! | Might, 2025

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This Wolf–Rayet star is called WR 31a, situated about 30,000 light-years away within the constellation of Carina. The outer nebula is expelled hydrogen and helium, whereas the central star, probably fusing carbon-or-heavier components in its core, burns at over 100,000 Ok. In very large, sizzling stars comparable to this, radiation strain performs a significant function in holding the star up towards gravitational collapse. However for Solar-like stars, fusion performs solely a minor function within the measurement, temperature, and brightness of the star. (Credit score: ESA/Hubble & NASA; Acknowledgement: Judy Schmidt)

All stars shine as a consequence of an inner supply of power. Often, it’s nuclear fusion: changing mass into power. What makes them most brilliant?

Ethan Siegel

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