Roughly speaking, naked singularities are singularities that may be se
en by timelike observers. The Cosmic Censorship conjecture forbids the
ir existence by stating that a reasonable system of energy will not, u
nder reasonable conditions, collapse into a naked singularity. There a
re however many (classical) counter-examples to this conjecture in the
literature. We propose a defense of the conjecture through the quantu
m theory. We will show that the Hawking effect and the accompanying ba
ck reaction, when consistently applied to naked singularities in two-d
imensional models of dilaton gravity with matter and a cosmological co
nstant, prevent their formation by causing them to explode or to emit
radiation catastrophically. This contrasts with black holes which radi
ate slowly. If this phenomenon is reproduced in the four-dimensional w
orld, the radiation accompanying the formation of naked singularities
should have observable consequences.