 |
Chemistry
Interstellar Inspiration
After
extensive research on living organisms, chemistry is now looking to
another vast source of inspiration: outer space. CNRS researchers have
already managed to reproduce, on Earth, one of the molecules most
commonly observed among the stars. This has led, in turn, to a whole
spectrum of new applications.
French scientists working in the US have recently managed to produce on Earth a substance that only exists in outer space.1
Guy Bertrand and his team at the Joint Research Chemistry Laboratory
(an international joint unit between CNRS and the University of
California, Riverside), specialize in producing molecules that are too
“unstable” to survive on our planet for more than a very brief period
of time. Their latest achievement is to have synthesized and then
isolated a strange material, that until now has only been detected in
interstellar space: “cyclopropenylidene carbene.” And this space
molecule already has a bright industrial future on Earth.
Nature
is such that chemists are not always able to confine all the substances
they are capable of producing to test tubes. This is sometimes
explained by the extreme “reactivity” of the products that are
generated: Certain molecules have an unfortunate tendency to combine
with their neighbors as soon as they are formed. Consequently, they
disappear very quickly from the test tube, as is the case with
“carbenes.” Unlike what happens with better-known organic molecules
like methane (CH4), “carbenes” do not have eight electrons surrounding
their carbon atoms but six, a deficit which according to the laws of
chemistry, leads to very high reactivity.
Cyclopropenylidene
(C3H2) is also affected by this rule. On Earth, this carbene–made up of
three carbon atoms arranged in a triangle with two hydrogen atoms
attached–only survives for a fraction of a second at best before
reacting with a surrounding molecule and disappearing. However, in the
freezing and rarefied environment of outer space, where intermolecular
combinations are rare, it can survive for quite a long time in its
normal state. First spotted in 1985, C3H2 is now considered one of the
most abundant organic substances found in space to date. Apart from
being observed in galaxies, astronomers have also detected it within
interstellar molecular clouds.
Bertrand
and his colleagues could not ignore such a prominent space dweller and
set up their laboratory five years ago to “prepare, under normal
conditions, molecules considered unstable.” They have had several
“impossible” successes such as the stabilization, four years ago, of a
“diradical,” a molecule with a promising future in the preparation of
organic magnets.2
To
curb the particularly reactive nature of cyclopropenylidene and create
a stable version of the molecule, the research team replaced the two
atoms of hydrogen by two “amino” groups, in other words compounds
containing one atom of nitrogen and two other identical atoms (NR2).
But why go to such trouble? “Many molecules that have applications in
everyday life are derived from natural substances,” explains Bertrand.
“Until now, researchers have been inspired by molecules that exist on
our planet. Why not look beyond?” And these efforts have already been
rewarded. “Our first results on cyclopropenylidene, partially funded by
the chemical firm Rhodia, show that this carbene could be used to
activate organometallic catalysts or even act as a catalyst itself.”
Vahé Ter Minassian
1.
V. Lavallo, et al., “Cyclopropenylidenes: from interstellar space to an
isolated derivative in the laboratory,” Science. 312 (5774): 722-4.
2006.
2. D. Scheschkewitz, “Singlet diradicals: from transition states to crystalline compounds,” Science. 295 (5561): 1880-1. 2002.
1. Consult the web site
|
 |