In microgravity, crystals of semiconductors and proteins can be grown
with improved crystallinity, offering the prospect of improved structu
ral analyses (for proteins) and better electronic properties (for semi
conductors)(1-3). Here we study the effect of a microgravity environme
nt on the crystallization of a class of materials-layered microporous
tin(IV) sulphides(4-11)-whose crystal structure is determined by weak
interlayer interactions (electrostatic, hydrogen-bonding and van der W
aals) as well as strong intralayer covalent bonds. We find that the cr
ystals grown in microgravity (on board the Space Shuttle Endeavour) sh
ow improved crystal habits, smoother faces, greater crystallinity, bet
ter optical quality and larger void volumes than the materials grown o
n Earth. These differences are due at least in part to the profound in
fluence of microgravity on the layer registry over length scales of ar
ound a nanometre, which is shown by X-ray and electron diffraction to
be better in space than on Earth. Thus we can see a clear distinction
between the covalent bonds in these materials, which are not significa
ntly affected by microgravity, and the weaker forces (like those that
determine the structure of proteins over length scales of around 0.3-0
.4 nm) which are more susceptible to the dynamic disturbances that ope
rate in crystallization on Earth.