
22.1 Preview 1125
There exists no better thing in the world than beer to blur class and social
differences and to make men equal.
—EMIL FISCHER
1
22.1 Preview
In the preceding chapter, we encountered neighboring group effects, the influence of
one functional group on the chemistry of another. In this chapter, we discuss mol-
ecules that bristle with functionality, and for which intramolecular neighboring group
effects play most important roles, influencing both structure and reactivity.These are
the carbohydrates, which are molecules that have the formula of C
n
H
2n
O
n
.The name
carbohydrate comes from the formulas of these compounds, which can be factored
into C
n
(H
2
O)
n
.These molecules appear to be hydrates of carbon. Of course they are
not literally hydrates,which are compounds having water molecules clustered around
an atom,but the classic demonstration experiment in which a carbohydrate sample—
usually a sugar cube—is treated with sulfuric acid does yield a spectacular sight as
exothermic dehydration reactions produce steam and a cone of carbon.
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Carbohydrates
are also called sugars or saccharides.
Carbohydrates serve as the storage depots for the energy harvested from the
sun through photosynthesis by green plants. Moreover, carbohydrates are present in
nucleic acids (Chapter 23) and are thus vital in controlling protein synthesis and in
transmission of genetic information.Table sugar is a carbohydrate.More than 100 mil-
lion tons of this sugar are produced yearly, and each American consumes about 64 lb
of table sugar per year (down from over 100 lb just a few years ago). Carbohydrates
are vital to human survival,and it is somewhat surprising that their study took so long
to emerge as a glamorous area of research. Perhaps the development of carbohydrate
chemistry was delayed by the simple technical difficulties of working with goopy syrups
rather than nice, well-behaved solids. A full scale renaissance is underway now, how-
ever, and carbohydrate chemistry is very much a hot topic.
3
The carbohydrate chemistry we will see in this chapter involves only a few new
reactions, but the polyfunctionality of these compounds can make for some com-
plications. To understand carbohydrate transformations you will have to be able to
apply old reactions in new settings, and work with a good deal of stereochemical
complexity as well. It’s not a bad idea to review the concepts in Chapter 4 before
you start on this chapter.That’s a hard thing to do—time is probably pressing,and it’s
always more interesting to move on to new stuff—but at least reread the summary
sections of Chapter 4 and be prepared to look back if things get confusing. Dust off
your models. There will be moments when they will be essential.
In this chapter, we will also meet Emil Fischer (1852–1919) again. He is surely
one of the greatest of organic chemists and a person of heroic theoretical and exper-
imental achievements. Carbohydrates can be hideously frustrating molecules to work
with experimentally. They form syrups and are notoriously difficult to crystallize.
1
Emil Fischer (1852–1919) was perhaps the greatest of all organic chemists. He won the 1902 Nobel Prize
in Chemistry and made extraordinary contributions to many fields, including the chemistry of carbohydrates
and proteins.
2
DO NOT try this experiment unsupervised! The reaction is very exothermic and sometimes violent. Sulfuric
acid can be thrown about, and sulfuric acid in the eyes is no picnic!
3
Although commercial sugars are mostly harvested from plants (mainly sugar beets or sugarcane), there are some
marvelously exotic laboratory syntheses. One favorite is that of Philip Shevlin (b. 1939) of Auburn University,
who fired bare carbon atoms into water and obtained carbohydrates. Shevlin has suggested that this reaction
may well have occurred on the icy surfaces of comets, transforming them into giant orbiting sugar cones.