The discussion focuses on proving the moment of inertia for a thin-walled hollow sphere using Cartesian coordinates instead of polar coordinates. The initial equation y^2 + x^2 = r^2 is clarified as representing a circle, not a sphere. A surface integral is proposed to calculate inertia, specifically 8ρ∫∫√(x^2 r^2/(r^2 - x^2 - y^2)) dy dx, with the suggestion to evaluate it for one octant and multiply by eight due to symmetry. The setup of the integral is based on the definition of inertia, which involves integrating the distance squared times mass. A correction is noted regarding the integral, indicating that x^2 should actually be x^4 inside the square root.