A review is given of this new and fascinating branch of chemistry,
starting with the detection, several years ago, of NH/sub 3/, H/sub 2/O, and HCHO
in interstellar space. Since then, with the advent of better radiotelescopes,
about 20 other small molecules have been identified. Questions discussed
include: how many more of these molecules exist, how are they formed, what sort
of reactions
... [Show full abstract] do they undergo, and were they of any significance in the origin of
life. It is certain, however, that under galactic conditions the chemistry of
these molecules is very different from that on Earth. (UK)