Figuring out mass of a star based on diameter

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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

[tex]R=M^{.8}[/tex]

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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