  We have completed a systematic survey for disks around young brown dwarfs and
very low mass stars. By choosing a well-defined sample and by obtaining
sensitive thermal IR observations, we can make an unbiased measurement of the
disk fraction around such low mass objects. We find that ~75% of our sample
show intrinsic IR excesses, indicative of circum(sub)stellar disks. We discuss
the physical properties of these disks and their relation to the much better
studied disks around solar-mass stars. The high incidence of disks around
substellar objects also raises the possibility of planetary systems around
brown dwarfs.
