Editing Black hole (section)

=== Ergosphere ===
{{Main|Ergosphere}}
[[File:Ergosphere and event horizon of a rotating black hole (no animation).gif|thumb|The ergosphere is a region outside of the event horizon, where objects cannot remain in place.<ref name=viss>{{cite arXiv |eprint=0706.0622 |last1=Visser |first1=Matt |title=The Kerr spacetime: A brief introduction |class=gr-qc |year=2007 |at=page 35, Fig. 3}}</ref>]]

Rotating black holes are surrounded by a region of spacetime in which it is impossible to stand still, called the ergosphere. This is the result of a process known as [[frame-dragging]]; general relativity predicts that any rotating mass will tend to slightly "drag" along the spacetime immediately surrounding it. Any object near the rotating mass will tend to start moving in the direction of rotation. For a rotating black hole, this effect is so strong near the event horizon that an object would have to move faster than the [[speed of light]] in the opposite direction to just stand still.<ref>{{harvnb|Carroll|2004|loc=Ch. 6.6}}</ref>

The ergosphere of a black hole is a volume bounded by the black hole's event horizon and the ''ergosurface'', which coincides with the event horizon at the poles but is at a much greater distance around the equator.<ref name=viss />

Objects and radiation can escape normally from the ergosphere. Through the [[Penrose process]], objects can emerge from the ergosphere with more energy than they entered with. The extra energy is taken from the rotational energy of the black hole. Thereby the rotation of the black hole slows down.<ref>{{harvnb|Carroll|2004|loc=Ch. 6.7}}</ref> A variation of the Penrose process in the presence of strong magnetic fields, the [[Blandford–Znajek process]] is considered a likely mechanism for the enormous luminosity and relativistic jets of [[quasars]] and other [[active galactic nuclei]].