Sommerville (1922) described four space-filling tetrahedra in Euclidean space. Goldberg (1974) subsequently noted five individual cases in the literature and added three
infinite families. Three of Sommerville's examples had previously been described
by Hill (1895). Baumgartner (1968) later independently rediscovered three and found
an additional example (Eppstein et al. 2004).
In the complete classification of rational tetrahedra (Kedlaya et al. 2020), all members of the first (Hill) one-parameter family
are space-filling. The second family contributes no additional space-fillers, since
its only space-filling member at also belongs to the first family. Chentouf and Sun (2023)
also ruled out 19 of the 59 sporadic rational tetrahedra, leaving at most 40 as possible
space-fillers.
Among unit-volume tetrahedra that tile Euclidean space, Sommerville type 4v has the least surface area (Bongiovanni et al. 2020).
An interactive visualization of space-filling tetrahedra is given by Pegg (2010).
The five panels illustrated below show fixed representatives traditionally named Sommerville Nos. 1-4 and Baumgartner T3. In each panel, the orange tetrahedron
at left is the seed and the multicolored solid at right is a triangular
prism, parallelepiped, cube,
or oblique triangular prism assembled from congruent copies.
In the numbering used by Pegg (2023), sporadic rational tetrahedron No. 2 is congruent to Sommerville No. 2. It can be represented by the vertices,
,
,
and .
Its dihedral angles along edges , , , , , and are , , , , , and , respectively.