The canonical hole set for non-metallic solids has been defined in ord
er to provide a more specific and quantitative description of the inte
rstitial structure of non-crystalline solids. Although a broad set of
construction criteria would allow an indefinitely large number of poly
hedra, considering regular-faced convex polyhedra, prisms, and antipri
sms, the canonical hole set for non-metallic solids is a total of 126
polyhedra. As expected, this number is substantially larger than the t
otal of eight Bernal holes for metallic solids. An even more compact s
et for non-metals (28 convex polyhedra and 16 prisms and antiprisms) i
s possible by considering only 'simple' polyhedra which can not be fur
ther dissected. A simple application of this approach is the descripti
on of cristobalite, a crystalline analog for vitreous silica, in which
the interstices are relatively undistorted truncated tetrahedra. A su
bstantially more complex application is the description of wollastonit
e, a crystalline analog for CaSiO3, glass, in which the interstices ar
e relatively distorted tetrahedra, square pyramids, and triangular pri
sms.