Relative atomic mass rounded to the nearest integral value equals the atomic mass number A. Thus, ignoring the masses of the atomic electrons and binding energies, nuclear mass expressed in unified atomic mass unit = A u. Also, it is experimentally found that the volume of a nucleus is directly proportional to the mass number A. As both nuclear mass and volume are proportional to the mass number, nuclear density is essentially the same for all nuclei.
Number volume = \(\cfrac43\)πR03A
∴ Nuclear density, \(\rho\) = \(\cfrac{nuclear\,mass}{nuclear\,volume}\)

Substituting the value of R0 in Eq.(1),

The order of nuclear density is 1017 kg/m3.
[Note : Some stars, with masses between 1.4 M⊙ and 3 M⊙, where M⊙ denotes the mass of our Sun, undergo supernova at the end of their active life and collapse into neutron stars of densities comparable with nuclear v density.]