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Im no astrophysicist but an older star would consume more of its hydrogen over time in comparison to helium through its fusion process. Over time concetrations would change resulting in a higher helium to hydrogen ratio.

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Osvaldo Runte

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Q: Why would an older main sequence star composed of a higher percentage of helium than a young main-sequence star?
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What old-main-sequence star will be composed of a higher percentage of helium than a young main-sequene star?

All of them, that's how a star gets to be "old" ... it converts its hydrogen into helium.


Why would an older main sequense star be composed of a higher percentage of helium than a young main sequence star?

A star's nuclear fusion reaction converts hydrogen into helium, and generates energy through this process. A "new" star has a fairly low percentage of helium, but over the course of billions of years, it fuses the hydrogen "fuel" into helium "ash".


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Cecilia Payne discovered that stars in the main sequence of development are composed almost entirely of the elements hydrogen and helium, which contradicted the current beliefs of the time.


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Most stars - and specifically main-sequence stars - get their energy from converting hydrogen-1 to helium-4, so you would expect that the percentage of hydrogen will decrease over time, while the percentage of helium would increase over time. Please note that the rate of fusion depends a LOT on the mass of the star; so you might have a very massive star that's only a few million years old and has already burned up most of its fuel (hydrogen), and another star, a red dwarf, that's 10 billion years old and has only used a small percentage of its fuel.


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