In the discussion about obtaining the velocity vector in a 3D spherical coordinate system, participants clarify that the time derivative must include all components: radial, polar angle, and azimuthal angle. The velocity vector is expressed as v = (dr/dt)hat{r} + r(dθ/dt)hat{θ} + r sin(θ)(dφ/dt)hat{φ}. There is a focus on the importance of considering the nature of the system, as the angles θ and φ may not always be invariant over time. Additionally, the position vector is confirmed to be solely radial, represented as rhat{r}, since θ and φ are angular measures, not distance. The conversation emphasizes the correct formulation of the velocity vector in spherical coordinates.