Figuring out mass of a star based on diameter

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The mass of a star can be estimated from its diameter using the equation R=M^{0.8} for main sequence stars, where R represents diameter. However, this relationship does not apply to non-main sequence stars, such as red giants and supergiants. For example, while the Sun's mass remains constant as it expands into a red giant, its radius significantly increases. Similarly, Betelgeuse has a mass 14 times that of the Sun but a radius 630 times greater. Understanding these distinctions is crucial for accurately determining stellar mass across different types of stars.
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How do you find the mass of a star based on its diameter? are there other factors that play into it and other things like that or is it just an equation?
 
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For main sequence stars you can use

R=M^{.8}

with R being the diameter. For non-main sequence stars, this doesn't hold however. For instance, when our Sun expands into a red giant, its mass will not increase but its radius will do so greatly. Another Example is Betelgeuse, a super giant with a mass 14 times that of the Sun and a radius 630 times as much.
 
i can figure out that non main sequence stars hold the same mass because its just less matter per square mile or sqaure yoctometer or whatever measure u want to use.
 
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