A star cluster contains N stars, each of mass m, with total mass M and radius R. The density decreases as 1/r^2 from the center. The document asks to: 1) Derive an expression for the total kinetic energy of the stars in terms of the radial velocity dispersion σR, mass and/or radius. 2) Derive an expression for the internal energy U as a double integral of the mass and radius. 3) Use the results to derive the Virial mass as M=3GR^2/σR^2.