Assuming you know the core mass, and other data about the sun, such as temperatures and pressures. Find the density at the very center of a star.
I think this may be involved.
P(r) = p(r)/µmH kT(r)
The Attempt at a Solution[/B]
I don't know where to begin with this. I tried changing the equation to make density the subject, but when I plug figures in I seem to be way off. I thing I maybe going down the wrong path.