This essay reviews recent developments in the theory of Hawking evapor
ation of black holes. Study of near extremal magnetically charged blac
k holes using a two plus four dimensional effective field theory has l
ed to the concept of homed particles or cornucopion as the endpoint of
Hawking evaporation. Horned particles are geometries containing two l
arge asymptotic regions connected by microscopic necks. They look like
point particles to an observer in any given asymptotic region, but in
many ways behave like macroscopic objects. In particular, it is very
difficult to pair produce them in external fields and their contributi
on to virtual loops is highly suppressed. They can serve as the remnan
ts necessary to account for the information apparently lost in Hawking
evaporation. The information simply goes into the new asymptotic regi
on formed when the black hole collapses and evaporates.