Calculate the density at the centre of the Sun

AI Thread Summary
To calculate the density at the center of the Sun, one must consider core mass, temperature, and pressure data. The equation P(r) = p(r)/µmH kT(r) is relevant, but there is confusion regarding rearranging it to solve for density. Attempts to isolate density have led to incorrect results, indicating a potential misunderstanding of the variables involved. Clarification on the definitions of these variables is necessary for accurate calculations. Understanding the relationships between pressure, temperature, and density is crucial for solving this problem effectively.
artworkmonkey
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Homework Statement


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.

Homework Equations


I think this may be involved.

P(r) = p(r)/µmH kT(r)

The Attempt at a Solution

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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.
 
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I rearrange the equation to be p(r)=µmHP(r)/kT(r)
maybe this is not the right equation.
 
artworkmonkey said:

Homework Equations


I think this may be involved.

P(r) = p(r)/µmH kT(r).
Impossible to say without knowing how all those variables defined.
 
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