We present high resolution, 2-D, near-infrared (J to L bands) images of the
young stellar object HL Tau, taken with an infrared camera. These images
show that light from the central young star scatters off a surrounding
thick (geometrically flaring) disk. The disk is tilted by 20-30 toward the line of sight. The disk's
radius is
500 AU and its mass is
at least 0.01-0.1 M
depending on
grain composition.