Bianchi models and Kantowski-Sachs models are both homogeneous and isotropic cosmologies, but they differ in their symmetry groups. Bianchi models have a 3-parameter symmetry group, indicating a simple transitive action where one symmetry operation maps any point to another without further rotation. In contrast, Kantowski-Sachs models feature a 4-parameter symmetry group, allowing for rotations about a fixed axis, thus making the symmetry multiply transitive. The distinction lies in the nature of their symmetry operations, with Bianchi being anisotropic and Kantowski-Sachs incorporating additional rotational symmetry. This understanding clarifies the mathematical definitions and implications of these cosmological models.