
526 CHAPTER 12 Dienes and the Allyl System: 2p Orbitals in Conjugation
About 70 years ago, structure determination was an entire branch of chem-
istry. People spent whole careers working out the structures of complicated
molecules by running chemical reactions. The products of many reactions of an
unknown compound were analyzed and inferences were made regarding the
structure of the unknown. This task was time-consuming and extraordinarily
demanding of experimental technique, intellectual rigor, and the development,
over years of work, of an intuitive sense of what was right, of what a given exper-
iment might mean. In a way, this work had all the satisfactions and charms of
handwork, of a craft. Nowadays, the work of years can usually be done in hours,
and chemists attack structural problems that would have been beyond any chem-
ical determination. Spectroscopy has made the difference. First came the devel-
opment of ultraviolet/visible (UV/vis) spectroscopy. We will deal with that
subject in this chapter. Then followed infrared (IR) spectroscopy and finally
nuclear magnetic resonance (NMR). The power of NMR is so great that this
technique has largely eclipsed all other forms of structure determination. We
introduced NMR spectroscopy in Section 2.14, and we will devote much of
Chapter 15 to this subject.
The development of spectroscopy certainly brought progress, and no reasonable
person would want to turn back the clock to the days of hand-crafted structure deter-
mination. Yet, one can sympathize with the feeling that there has been some loss
with the progress. We are somehow not as close to the molecules as we once were,
even though we know much more about them. There is a psychological distance
involved here. One tends to believe what spectrometers say and to read too much
into the data. In chemistry, nothing is more important than honing one’s critical
sense.It is somehow easier to ignore some small, but ultimately vital glitch on a piece
of chart paper than to ignore the results of an experiment gone in an unexpected
direction. The former somehow melts into the noise of the baseline, while the lat-
ter teases the imagination.
One can also sympathize with those practitioners of the art of structure
determination who saw the future when the first NMR machine was delivered,
and realized that for them, “NMR” meant “No More Research.” They were
right.
Ultraviolet/visible spectroscopy is called electronic spectroscopy because it deals
with the absorption of energy by electrons in molecules. The energy absorbed (¢E)
is used to promote an electron from one orbital to a higher-energy orbital (Fig. 12.25).
The magnitude of ¢E is proportional to the frequency of the light, ν, and inversely
proportional to wavelength of the light, λ, as shown by
¢E hν hc/λ (12.1)
where h is Planck’s constant and c is the speed of light. Because electrons are restrict-
ed to orbitals of specific energy, ¢E is also quantized and may have only certain values.
The distinction between ultraviolet and visible spectroscopy is an artificial one and
is based solely on the fact that the detectors built into our bodies, our eyes, are sensi-
tive only to radiation of wavelength 400–800 nm (nm nanometers; 1 nm 10
9
m),
which we call the visible spectrum. Spectrometers are less limited in this respect than
we are, and UV spectrometers easily detect radiation from 200–400 nm, as well as the
entire visible range and beyond. At higher energy, below 200 nm, the atmosphere begins
to absorb strongly, and spectroscopy in this range is more difficult, although by no
means impossible.
Energy
LUMO
HOMO
⌬E =h
ν
FIGURE 12.25 Absorption of UV
light promotes an electron from the
HOMO to the LUMO.