Figure 14-11 Structure of a Kerr (Rotating) Black Hole Rotating black holes are only slightly more complex than non-rotating ones. The singularity of a kerr black hole is located in an infinitely thin ring around the center of the hole. The ring appears as an arc in this cutaway drawing. The event horizon is again a spherical surface. There is also a doughnut-shaped region, called the ergoregion, just outside the event horizon, in which nothing can remain at rest. Space in the ergoregion is being curved or pulled around by the rotating black hole.