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3: UV Spectroscopy

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    332803
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    UV Spectroscopy

    Which electrons can be excited? Where do they go?

    In order to absorb UV-Vis light, the molecule must contain a chromophore—the part of a molecule that absorbs UV light.

    An MO diagram for formaldehyde (methanol, CH2O) is shown.

    clipboard_e3a979463808ef1ba691e5cdfd71e4f34.png

    • Place the proper number of electrons in the diagram.

    There are 4 common types of transitions (n-\(\pi\)*, \(\pi\)-\(\pi\)*, \(\sigma\)-\(\sigma\)*, n-\(\sigma\)*) for organic compounds

    • What structural features must be present for each type of transition?
      • \(\sigma \rightarrow \sigma\)*
      • \(\pi \rightarrow \pi\)*
      • \(n \rightarrow \pi\)*
      • \(n \rightarrow \sigma\)*
    • Propose transition types for the list of functional groups below:
      • Alkane
      • Alkene
      • Alkyne
      • Alcohol
      • Carbonyl
      • Amine
      • Nitrile
    • Molecules with chromophores tend to have a lot of pi bonds. Explain why.

     

    Table of wavelengths and extinction coefficients (\(\epsilon_{max}\)) for those transitions
    Transition ~\(\lambda_{max}\) (nm) \(\epsilon_{max}\)
    \(\sigma \rightarrow \sigma\)* 135 v. small
    \(\pi \rightarrow \pi\)* 160-280 2,400-25,000
    \(n \rightarrow \pi\)* 279-320 10-50
    \(n \rightarrow \sigma\)* 160-250 100-7,000
    • Why are the \(\lambda_{max}\) values shown as ranges and not discrete numbers?
    • Using the MO energy diagram, explain the relative energies of the transitions.

    clipboard_e7a3db78a14e06ecc2ce5d25da4ba9365.png

     

    Extinction Coefficients

    Beer’s law states that the absorbance of a solution is proportional to its concentration. Mathematically, Beer’s law is

    \[A = \epsilon b c\]

    A is the absorbance of the solution

    \(\epsilon\) is the quantity called the molar absorptivity

    b is the path length in cm of the solution cell

    c is the solution concentration (molarity)

    Absorbance spectra are usually gathered as a function of wavelength. Absorbance is dependent upon concentration.

    • Suppose that a UV absorbance spectrum was obtained for a solution of a compound. Then the concentration of the solution was doubled. Redraw the new spectrum on the same scale.

    clipboard_e5232100e26909f6f3846e3971be01d76.png

    Absorbance is also dependent the molar absorptivity. Molar absorptivity (\(\epsilon\)) tells you how likely an electronic transition is.

    • The more likely a particular absorbance occurs, then the [ smaller / larger ] the \(\epsilon\) will be.
    • If an electronic transition is difficult, _______ [ more / fewer ] electrons will be excited, and the \(\epsilon\) will ________ [ decrease / increase ] and the apparent intensity will be weaker.
    • \(\sigma \rightarrow \sigma\)* has a small extinction coefficient. Why?
    • \(n \rightarrow \pi\)* are the lowest energy of any transitions we observe and consequently have the longest wavelength. However, they typically have the smallest extinction coefficient. Why is the \(n \rightarrow \pi\)* transition so difficult even though the energy gap is small? Consider how much orbital overlap is present.

    clipboard_ee5f83c565b1cc816a8ab937809628fcb.png

    UV Spectroscopy: Analysis

    UV-Vis Spectroscopy is useful in the laboratory for several purposes.

    1. Determination of structure.
    2. Determination of the concentration of a known sample

    UV-Vis Spectroscopy: Determination of structure

    The molecules most likely to absorb light in the UV-Vis region are structures with pi bonds. This severely limits the use of UV-Vis as a general method for determining structure.

    Additionally, molecules with an isolated alkene tend to have \(\lambda_{max}\) around 170-190 nm which is not measure by most instruments.

    • With conjugation, the \(\pi \rightarrow \pi\)* orbitals are [ closer or further ] apart.

    clipboard_e729ab32582a0126293da206a301de469.png

    • Conjugated systems require [ higher or lower ] energy to excite an electron.
    • However, generally moves the absorption maxima to [ longer or shorter] wavelengths.

    Thus, conjugation becomes the major structural feature identified by this technique.

     

    Determination of Structure: Predicting \(\lambda_{max}\) of Conjugated Compounds There are some standardized rules for predicting the \(\lambda_{max}\) in conjugated molecules called the Woodward-Fieser Rules.

    Core Chromophore Substituent Influence

    Trans diene: 215 nm

    clipboard_e56354fe86eff2249a6e81d22a7a70e34.png

    Alkyl +5
    Alkoxy +6
    Halide +10

    Cis diene: 260 nm

    clipboard_ead6281990cd592583018c4fbc9a424f2.png

    Acyl 0
    Amino 60
    Another double bond +30
    Phenyl +60

    *Each exocyclic double bond adds 5 nm.

     

    • Predict the have \(\lambda_{max}\) for the following compounds.

    clipboard_e0cc86e26e3cd41fd27226d3fdd7db9f8.png

    Base (cis or trans): _______

    5 alkyl group substituents _______

    2 exocyclic bonds _______

    Additional double bond _______

    Total: _______ Compare to actual: 283 nm

     

    clipboard_e43b3795eee9c6a5ad43df599c20e2b69.png

    Base (cis or trans): _______

    4 alkyl group substituents _______

    2 exocyclic bonds _______

    Additional double bond _______

    Total: _______ Compare to actual: 355 nm

     

    Determination of Structure:

    Predicting \(\lambda_{max}\) of Conjugated Carbonyl Compounds The Woodward-Fieser Rules also extend to conjugated carbonyl compounds.

    Core Chromophore Substituent \(\alpha\)-Influence \(\beta\)-Influence

    Acyclic enone: 215 nm

    clipboard_e0f7ca4cd3d5a8defe466bd39631a3529.png

    Alkyl +10 +12
    Alkoxy/Hydroxyl +35 +30

    Cyclic hexenone: 215 nm

    clipboard_e144a11c19832d3c49df1915c2139d5d1.png

    Chloro +15 +12
    Bromo +25 +30
    Acyl +6 +6

    Cyclic pentenone: 202 nm

    clipboard_e5d4c61aa6c43ce0427630e8c572f904d.png

    Another double bond +30  
    Phenyl +60  

    *Each exocyclic double bond adds 5 nm.

    ** In water, add 8 nm.

    • • Predict the have \(\lambda_{max}\) for the following compounds.

    clipboard_ebc550a19eead18955bd8fffc8736e114.png

    Base (cis or trans): _______

    1 alpha alkyl group substituents _______

    2 beta alkyl group substituents _______

    Additional double bond _______

    Total: _______ Compare to actual: 249 nm

    clipboard_ea781de51c4e8dcc247d84e7e9e805297.png

    Base (cis or trans): _______

    alpha bromo group substituents _______

    2 beta alkyl group substituents _______

    Additional double bond _______

    Total: _______ Compare to actual: 251 nm

     

    There are lots of tables for use in predicting values. There are also databases of known UV spectra for direct comparison.

     

    UV-Vis Spectroscopy: Determination of the concentration of a known sample

    Beer's Law: \(A = \epsilon b c\)

    A is the absorbance of the solution

    \(\epsilon\) is the quantity called the molar absorptivity

    b is the path length in cm of the solution cell

    c is the solution concentration (molarity)

    • Explain how you could determine the concentration of a sample using Beer’s Law. Show the math.

    The literature value of ε for 1,3-pentadiene in hexane is 26,000 (mol / L)-1cm-1 at its maximum absorbance at 224 nm. You obtain a 10 mL sample and take a UV spectrum in a cell with a 1 cm path length, finding that A224 = 0.850.

    • What is the concentration (molarity) of the solution? Show your work.
    • How many grams of 1,3 pentadiene (molar mass = 68 g/mol) are in the solution?

     

    UV Spectroscopy: Solvent Choices

    Solvents used for UV Spectroscopy Samples

    • What solvents (list solvents with structures) would interfere with UV analysis?
    Solvent Structure
    Acetic acid (AcOH) clipboard_e521d2d4308faae7df311901e95c97447.png
    Acetone clipboard_ed9362dfee4f39476d4ca229279a9732d.png
    Benzene (PhH) clipboard_e66b4d22c98166221f7f525a20df3098a.png
    tert-Butyl methyl ether clipboard_eb7e33ca1255552a4b69a0b4ec4228c29.png
    Chloroform clipboard_ec48494cd553c0d7c6cf59c62f9436e23.png
    Diethyl ether clipboard_e080af901badc8dbd4c47cf18dae9b9da.png
    Dimethyl formamide clipboard_e6a21f4aea7369c7d91d0024859469212.png
    Dimethyl sulfoxide (DMSO) clipboard_eeeb9d656081feb00055994f5e47b1a1e.png
    Ethyl acetate (EtOAc) clipboard_ec59380423bab322c82779474b809bc49.png
    Hexane clipboard_e1cff34ef7ea13a999298a91b2d09d220.png
    Octane clipboard_ea28bfe8dae4594a3362ae87ea80b1cfd.png
    Tetrahydrofuran (THF) clipboard_e2ce65742c4bee79fff991c4f4816d21e.png
    Toluene (PhMe) clipboard_edf412ac83b868edb9262eb3c61d7f6fb.png
    Water clipboard_e01d875548f589dad77401b5c078360e3.png

     

    • Not everything is soluble in hexane/octane, what range of wavelengths can you measure using methanol as your solvent?

     

    Practice Problem

    1. It is often important to be able to quantify the amount of protein in a solution. One method is based on the fact that aromatic amino acids tyrosine (Tyr) and tryptophan (Trp) absorb ultraviolet light maximally at ~280 nm. The amino acid cysteine does not absorb at this wavelength; however, two cysteines may react with each other to form a disulfide (S-S) linkage which is called cystine and this structural feature does. The general method is to just take a solution of unknown protein sample, stick it into a spectrophotometer, and read the A280.

    Based on a sample of measured molar extinction coefficient (ε) values for 80 proteins, the ε at 280 nm of a folded protein in water, ε(280), can best be predicted with this equation:

    \[\epsilon(@ 280) (\text{M$^{-1}$cm$^{-1}$}) = (\#Trp)(5,500) + (\#Tyr)(1,490) + (\#cystine)(125) \]

    Of course, it is necessary to know the structure of the protein so that the number of each type of amino acid residue can be entered into the equation.

    • Examine the equation and predict the type of absorption that each of the three amino acids in the equation undergoes at 280 nm.
    • Draw the side chains of these three amino acids.
    • Does this match your prediction? Explain.

    This page titled 3: UV Spectroscopy is shared under a not declared license and was authored, remixed, and/or curated by Kate Graham.

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