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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?
The mass of a star can be estimated based on its diameter using the equation R = M^{0.8} for main sequence stars, where R represents the diameter and M the mass. However, this relationship does not apply to non-main sequence stars, such as red giants and supergiants. For example, the Sun's mass remains constant as it expands into a red giant, while Betelgeuse, a supergiant, has a mass 14 times that of the Sun and a radius 630 times greater. Understanding these distinctions is crucial for accurate stellar mass calculations.
PREREQUISITESAstronomy students, astrophysicists, and anyone interested in understanding stellar mass and diameter relationships in different types of stars.