Active galactic nuclei (AGN) are generally accepted to be powered by t
he release of gravitational energy in a compact accretion disk surroun
ding a massive black hole(1,2); such disks are also thought necessary
to collimate the powerful radio jets seen in some AGN(3). The unifying
classification schemes for AGN further propose that differences in th
eir appearance can be attributed to the opacity of the accreting mater
ial, which may obstruct our view of the central region of some systems
. The popular model for the obscuring medium is a parsec-scale disk of
dense molecular gas(4), although evidence for such disks has been mos
tly indirect, as their angular size is much smaller than the resolutio
n of conventional telescopes. Here we report direct images of a parsec
-scale disk of ionized gas within the nucleus of NGC1068, the archetyp
e of obscured AGN. The disk is viewed nearly edge-on, and individual c
louds observed within the ionized disk are opaque to high-energy radia
tion, consistent with the unifying classification schemes. The project
ed axes of the disk and AGN are aligned, from which we infer that the
ionized gas disk traces the outer regions of the long-sought inner acc
retion disk.