  In classical gravity, nothing can escape from a black hole, not even light.
In particular, this happens for stationary black holes because their horizons
are null. We show, on the other hand, that the apparent horizon and the region
near r = 0 of an evaporating charged, rotating black hole are both timelike.
This implies that there exists a channel, via which classical or quantum
information can escape to the outside, as the black hole evaporates. Since
astrophysical black holes have at least some rotation, our results apply to all
black holes in nature. We discuss the implications of our result.
