Visible and Ultraviolet Spectroscopy<?xml:namespace prefix = o ns = "urn:schemas-microsoft-com:office:office" />
1. Background
<?xml:namespace prefix = v ns = "urn:schemas-microsoft-com:vml" /><?xml:namespace prefix = w ns = "urn:schemas-microsoft-com:office:word" />An obvious difference between certain compounds is their color. Thus, quinone is yellow; chlorophyll is green; the 2,4-dinitrophenylhydrazone derivatives of aldehydes and ketones range in color from bright yellow to deep red, depending on double bond conjugation; and aspirin is colorless. In this respect the human eye is functioning as a spectrometer analyzing the light reflected from the surface of a solid or passing through a liquid. We see sunlight (or white light) as uniform or homogeneous in color, it is actually composed of a broad range of radiation wavelengths in the ultraviolet (UV), visible and IR portions of the spectrum.
The component colors of the visible portion can be separated by passing sunlight through a prism, which acts to bend the light in differing degrees according to wavelength. EM radiation such as visible light is commonly treated as a wave phenomenon, characterized by a wavelength or frequency. Wavelength is defined as the distance between adjacent peaks (or troughs), and may be designated in m, cm or nm (10-9 meters). Frequency is the number of wave cycles that travel past a fixed point /unit of time, and is usually given in cycles/second, or hertz (Hz). Visible wavelength ranges from approx. 400 to 800 nm. The longest visible wavelength is red and the shortest is violet. Other common colors of the spectrum, in order of decreasing wavelength, may be remembered by the mnemonic: ROY G BIV. The wavelength will increases on moving from left to right.
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When white light
passes through or is reflected by a colored substance, a
characteristic portion of the mixed wavelengths is absorbed. The
remaining light will then assume the complementary color to the
wavelength(s) absorbed. This relationship is demonstrated by the
color wheel shown on the right. Here, complementary colors are
diametrically opposite each other. Thus, absorption of 420-430 nm
light renders a substance yellow, and absorption of 500-520 nm
light makes it red. Green is unique in that it can be created by
absoption close to 400 nm as well as absorption near 800
nm.
Early humans valued colored pigments, and used them for decorative purposes. Many of these were inorganic minerals, but several important organic dyes were also known. These included the crimson pigment, kermesic acid, the blue dye, indigo, and the yellow saffron pigment, crocetin. A rare dibromo-indigo derivative, punicin, was used to color the robes of the royal and wealthy. The deep orange hydrocarbon carotene is widely distributed in plants, but is not sufficiently stable to be used as permanent pigment, other than for food coloring. A common feature of all these colored compounds, displayed below, is a system of extensively conjugated pi-electrons.
2. The Electromagnetic Spectrum
The visible spectrum constitutes but a small part of the total radiation spectrum. Most of the radiation that surrounds us cannot be seen, but can be detected by dedicated sensing instruments. This EM spectrum ranges from very short wavelengths (including gamma and x-rays) to very long wavelengths (including microwaves and broadcast radio waves).
Energy of segment of the spectrum is proportional to its frequency.
3. UV-Visible Absorption Spectra
The visible region of the spectrum comprises photon energies of 36 to 72 kcal/mole, and the near UV region, out to 200 nm, extends this energy range to 143 kcal/mole. UV radiation having wavelengths less than 200 nm is difficult to handle, and is seldom used as a routine tool for structural analysis.
The energies noted above are sufficient to
promote or excite a molecular electron to a higher energy orbital.
Consequently, absorption spectroscopy carried out in this region is
sometimes called "electronic
spectroscopy". A diagram showing the various
kinds of electronic excitation that may occur in organic molecules
is shown on the left. Of the six transitions outlined, only the two
lowest energy ones (left-most, colored blue) are achieved by the
energies available in the 200 to 800 nm spectrum. As a rule,
energetically favored electron promotion will be from the
highest occupied molecular orbital (HOMO) to the
lowest unoccupied molecular orbital (LUMO), and
the resulting species is called an excited
state.
When molecules are exposed to light having an energy that matches a
possible electronic transition within the molecule, some of the
light energy will be absorbed as the electron is promoted to a
higher energy orbital. An optical spectrometer records the
wavelengths at which absorption occurs, together with the degree of
absorption at each wavelength. The resulting spectrum is presented
as a graph of absorbance (A) vs wavelength, as in the isoprene
spectrum shown below. Since isoprene is colorless, it does not
absorb in the visible part of the spectrum and this region is not
displayed on the graph. Absorbance usually ranges
from 0 (no absorption) to 2 (99% absorption), and is precisely
defined in context with spectrometer operation.
Because the absorbance of a sample will be proportional to the number of absorbing molecules in the spectrometer light beam (e.g. their molar concentration in the sample tube), it is necessary to correct the absorbance value for this and other operational factors if the spectra of different compounds are to be compared in a meaningful way. The corrected absorption value is called "molar absorptivity", and is particularly useful when comparing the spectra of different compounds and determining the relative strength of light absorbing functions (chromophores). Molar absorptivity (ε) is defined as:
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Molar Absorptivity, ε = A/ c l |
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(A= absorbance, c = sample concn m/l & l = length of light path through the sample in cm.) |
If the isoprene spectrum on the right was obtained from a dilute hexane solution (c = 4 * 10-5 moles per liter) in a 1 cm sample cuvette, a simple calculation using the above formula indicates a molar absorptivity of 20,000 at the maximum absorption wavelength. Indeed the entire vertical absorbance scale may be changed to a molar absorptivity scale once this information about the sample is in hand. Clicking on the spectrum will display this change in units.
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From the chart above it should be clear that the
only molecular moieties likely to absorb light in the 200 to 800 nm
region are pi-electron functions and hetero atoms having
non-bonding valence-shell electron pairs. Such light absorbing
groups are referred to as chromophores. A list of
some simple chromophores and their light absorption characteristics
is provided on the left above. The oxygen non-bonding electrons in
alcohols and ethers do not give rise to absorption above 160 nm.
Consequently, pure alcohol and ether solvents may be used for
spectroscopic studies.
The presence of chromophores in a molecule is best documented by
UV-Visible spectroscopy, but the failure of most instruments to
provide absorption data for wavelengths below 200 nm makes the
detection of isolated chromophores problematic. Fortunately,
conjugation generally moves the absorption maxima to longer
wavelengths, as in the case of isoprene, so conjugation becomes the
major structural feature identified by this technique.
Molar absorptivities may be very large for strongly absorbing
chromophores (>10,000) and very small if absorption is weak (10
to 100). The magnitude ofε reflects both the size of the
chromophore and the probability that light of a given wavelength
will be absorbed when it strikes the chromophore.
4. The Importance of Conjugation
A comparison of the absorption spectrum of
1-pentene, λmax
= 178 nm, with that of isoprene (above) clearly
demonstrates the importance of chromophore conjugation. Further
evidence of this effect is shown below. The spectrum on the left
illustrates that conjugation of double and triple bonds also shifts
the absorption maximum to longer wavelengths. From the polyene
spectra displayed in the center diagram, it is clear that each
additional double bond in the conjugated pi-electron system shifts
the absorption maximum about 30 nm in the same direction. Also, the
molar absorptivity (ε) roughly doubles with each new conjugated
double bond. Spectroscopists use the terms defined in the table on
the right when describing shifts in absorption. Thus, extending
conjugation generally results in bathochromic and hyperchromic
shifts in absorption.
The appearance of several absorption peaks or shoulders for a given
chromophore is common for highly conjugated systems, and is often
solvent dependent. This fine structure reflects not only the
different conformations such systems may assume, but also
electronic transitions between the different vibrational energy
levels possible for each electronic state. Vibrational fine
structure of this kind is most pronounced in vapor phase spectra,
and is increasingly broadened and obscured in solution as the
solvent is changed from hexane to methanol.
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Terminology for Absorption Shifts
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To understand why
conjugation should cause bathochromic shifts in the absorption
maxima of chromophores, we need to look at the relative energy
levels of the pi-orbitals. When two double bonds are conjugated,
the four p-atomic orbitals combine to generate four pi-molecular
orbitals (two are bonding and two are antibonding). This was
described earlier in the section concerning
diene chemistry. In a similar manner, the three double bonds of a
conjugated triene create six pi-molecular orbitals, half bonding
and half antibonding. The energetically most favorable π
__> π* excitation occurs from
the highest energy bonding pi-orbital (HOMO) to
the lowest energy antibonding pi-orbital
(LUMO).
The following diagram illustrates this excitation for an isolated
double bond (only two pi-orbitals) and, on clicking the
diagram, for a conjugated diene and triene. In each case the
HOMO is colored blue and the LUMO is colored magenta. Increased
conjugation brings the HOMO and LUMO orbitals closer together. The
energy (ΔE) required to effect the electron promotion is therefore
less, and the wavelength that provides this energy is increased
correspondingly (remember
λ = h • c/ΔE ).
Many other kinds of conjugated pi-electron systems act as chromophores and absorb light in the 200 to 800 nm region. These include unsaturated aldehydes and ketones and aromatic ring compounds. A few examples are displayed below. The spectrum of the unsaturated ketone (on the left) illustrates the advantage of a logarithmic display of molar absorptivity. The π __> π* absorption located at 242 nm is very strong, with an ε = 18,000. The weak n __> π* absorption near 300 nm has an ε = 100.
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Benzene exhibits very strong light absorption near 180 nm (ε > 65,000) , weaker absorption at 200 nm (ε = 8,000) and a group of much weaker bands at 254 nm (ε = 240). Only the last group of absorptions are completely displayed because of the 200 nm cut-off characteristic of most spectrophotometers. The added conjugation in naphthalene, anthracene and tetracene causes bathochromic shifts of these absorption bands, as displayed in the chart on the left below. All the absorptions do not shift by the same amount, so for anthracene (green shaded box) and tetracene (blue shaded box) the weak absorption is obscured by stronger bands that have experienced a greater red shift. As might be expected from their spectra, naphthalene and anthracene are colorless, but tetracene is orange.
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The spectrum of the bicyclic diene (above right) shows some vibrational fine structure, but in general is similar in appearance to that of isoprene, shown above. Closer inspection discloses that the absorption maximum of the more highly substituted diene has moved to a longer wavelength by about 15 nm. This "substituent effect" is general for dienes and trienes, and is even more pronounced for enone chromophores.
