It is suggested here that an alternative strategy for detecting signs of pr
ebiotic chemistry on Titan would be to search for stereoregular polymers. L
aboratory simulations of Titan's atmosphere suggest several interesting rea
ctive vinyl monomers, including acrylonitrile. Polyacrylonitrile and deriva
tives made by side chain modification would be very interesting structures
that could be envisioned as progenitors of complex chemical systems. The is
sues and challenges of considering polymer, rather than small molecule, ste
reochemistry as an indicator of prebiotic chemistry on Titan are briefly di
scussed.