bluejazz
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Homework Statement
Find the enclosed mass profile M(r) in terms of R* and the total mass M* of the star.
Homework Equations
dMr/dr = 4(pi)r2(density)
density is given as: rho(r) = (rho_c)[1-(r/R*)2]
Where rho_c is the central density and R* is the radius of the star.
3. Attempt at a solution
I plugged the given density into the enclosed mass formula, took the integral in terms of r, and ended up with the result:
M(r) = 4(pi)(rho_c)[r3/3 - r5/(5R*2)]
My problem is, I'm not sure how to put this in terms of Mstar. What I think is I have to take the central density and the expression for volume [4/3 * (pi) * r3] and get Mstar. I guess my real question is this: what is the definition of central density?