  Voids are the most prominent feature of the large-scale structure of the
universe. Still, they have been generally ignored in quantitative analysis of
it, essentially due to the lack of an objective tool to identify the voids and
to quantify them. To overcome this, we have developed the VOID FINDER
algorithm, a novel tool for objectively quantifying voids in the galaxy
distribution. We apply the algorithm to two redshift surveys, the dense SSRS2
and the full-sky IRAS 1.2-Jy. Both surveys show similar properties: ~50% of the
volume is filled by the voids. The voids have a scale of at least 40 h^{-1}Mpc,
and a -0.9 average under-density. Faint galaxies do not fill the voids, but
they do populate them more than bright ones. These results suggest that both
optically and IRAS selected galaxies delineate the same large-scale structure.
Comparison with the recovered mass distribution further suggests that the
observed voids in the galaxy distribution correspond well to under-dense
regions in the mass distribution. This confirms the gravitational origin of the
voids.
