To measure the mean density of a neutron star with a known mass of three solar masses, one can estimate its radius, typically around 12 kilometers. Using the formula for density, which is mass divided by volume, the volume can be calculated assuming a spherical shape. While the radius may vary among neutron stars, this estimate provides a reasonable basis for calculations. The mean density can then be derived from these parameters, highlighting the extreme density characteristics of neutron stars. Accurate measurements of mass and radius are crucial for understanding their properties.