The templated syntheses of TMA(2)Sn(3)S(7) and TBA(2)Sn(4)S(9) (where
TMA is tetramethylammonium and TEA is n-tetrabutylammonium) microporou
s layered tin(Iv) sulfides have been carried out under both microgravi
ty (mu G) and earth (1G) conditions in order to elucidate the influenc
e of gravity on the self-assembly and crystal-growth processes of this
class of materials. The mu G experiments were conducted on board the
May 1996 Endeavour STS-77 NASA space-shuttle flight. It was determined
that the long-range ordering of the porous layers and the population
of defects but not the short-range ordering within the layers is influ
enced by gravity. Bulk and surface crystallinity, smoothness of crysta
l faces, optical quality, crystal habits, registry of the porous layer
s, and accessible void volume to adsorbates were found to be improved
in the space-grown crystals. This is probably because the forces assoc
iated with the organization of the porous layers are expected to be we
ak and sensitive to the elimination of buoyancy-driven convective flow
s and Stokes sedimentation effects in a microgravity environment, One
can draw an analogy to the weak forces between protein macromolecules
and the established effect of microgravity on improving the diffractio
n quality of crystals harvested in space.