For a comparison, the core of the sun has 150g/cm³. The closest thing I could find was the stellar core of a star with 0.1 solar masses, which is 500g/cm³. Apparently the density in the core increases as mass decreases, at least for main sequence stars, the other stars seem to work differently and can get higher in another scale.
For a comparison, the core of the sun has 150g/cm³. The closest thing I could find was the stellar core of a star with 0.1 solar masses, which is 500g/cm³. Apparently the density in the core increases as mass decreases, at least for main sequence stars, the other stars seem to work differently and can get higher in another scale.