In a rotating disc, the angular velocity is uniform across the entire disc, including its center, denoted as ##\vec \omega##. While all points on the disc share the same angular velocity, their linear velocities vary based on their distance from the axis of rotation, with linear velocity defined as ##\vec v = \vec \omega \times \vec r##. When the position vector ##\vec r## is very small, such as at the Planck length, the linear velocity remains non-zero but minimal. The discussion clarifies that if angular velocity is constant, "tangential" and "linear" velocities are equivalent. The conversation also touches on the implications of non-classical physics in this context.