An embedding diagram helps visualize the observer-dependent projected spati
al geometry of the equatorial plane in the Kerr spacetime as Seen by a fami
ly of circularly rotating observers. This is described for the various geom
etrically defined families of such observers, motivated by the attempt to b
etter understand how the spatial geometry contributes to the properties of
particle motion as seen by those observers. A new family of observers is in
troduced for which the equatorial plane appears to be flat.