Calculate Star Mass from Radius: An Integration Approach

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The discussion centers on calculating the mass of a star using integration, specifically deriving the formula M = 4πp_c(R^3/3). The user initially struggles with the integration process to find the mass within a radius and contemplates using radial masses. They realize that substituting the total radius 'R' into their equation simplifies the problem. Ultimately, they conclude that the total mass can be derived from the average density and volume formula, M = ρV, where V is the volume of the star. The conversation highlights the importance of understanding the relationship between mass, density, and volume in astrophysics.
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Sorry no one was answering my question, and I just wanted to get this done:

Homework Statement


...Hence show that the mass of the star is M = 4\pip_{c}\left(R^{3}/3 )

Homework Equations


M(r) = 4 \pip_{c}\left(r^{3}/3 - r^{4}/4R)
This is the mass within a radius

The Attempt at a Solution


I already found the mass within a radius via intergration (look at relevant equations), and I know that I have to build up an 'infinite' number of radial masses to get the whole mass of the star. But do I use integration on this equation or something else? What do I do?
 
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Oohh for f_cks sake... I realized

Total radius of the star is 'R'. Just substitute that in for r and cancel, since r1 is subjective and doesn't factor for the whole star.

WHHHYYYYYY!??
 
The total mass of anything is just M=pV where p is the average density and V is the volume. Here V=4/3*pi*R^3. That's that...
 
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