  The Bohr-Sommerfeld quantization rule is useful to study the area spectrum of
black holes by employing adiabatic invariants. This method is extended to
charged dilaton black holes in 2+1 dimensions. We put the background space-time
into the Kruskal-like coordinate to find the period with respect to Euclidian
time. Also assuming that the adiabatic invariant obeys Bohr-Sommerfeld
quantization rule, detailed study of area and entropy spectrum has been done.
It is dependent on the charge and is equally spaced as well.
  We also investigate the thermodynamics of the charged dilaton black hole.
