  Dust plays a central role in the unification theory of active galactic nuclei
(AGNs). However, little is known about the nature (e.g., size, composition) of
the dust which forms a torus around the AGN. In this Letter we report a
systematic exploration of the optical extinction (A_V) and the silicate
absorption optical depth (\Delta\tau9.7) of 110 type 2 AGNs. We derive A_V from
the Balmer decrement based on the Sloan Digital Sky Survey data, and
\Delta\tau9.7 from the Spitzer/Infrared Spectrograph data. We find that with a
mean ratio of A_V/\Delta\tau9.7 ~ 5.5, the optical-to-silicate extinction
ratios of these AGNs are substantially lower than that of the Galactic diffuse
interstellar medium (ISM) for which A_V/\Delta\tau9.7 ~ 18.5. We argue that the
anomalously low A_V/\Delta\tau9.7 ratio could be due to the predominance of
larger grains in the AGN torus compared to that in the Galactic diffuse ISM.
