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Chapter 13 Structure Determination

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Title: Chapter 13 Structure Determination


1
Chapter 13 Structure Determination

2
Four of the most useful techniques

3
13.1 Electromagnetic Radiation A Common
Probe of Structure
FIGURE 13.1 The electromagnetic spectrum.
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Chapter 13. Structure Determination
4
FIGURE 13.2 (a) Wavelength (?) is the distance
between two successive wave maxima. Amplitude is
the height of the wave measured from the center.
(b)(c) What we perceive as different kinds of
electromagnetic radiation are simply waves with
different wavelengths and frequencies.
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Chapter 13. Structure Determination
5
13.2 X-Ray Crystallography
FIGURE 13.3 The structure of arachidonic acid
and cyclooxyge-nase as determined from X-ray
crystallography. (Dr. Lisa M. Perez, Texas AM
University. Used with permission.)
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Chapter 13. Structure Determination
6
FIGURE 13.4 The steps required to perform a
structure determina-tion using X-ray
crystallography include obtaining crystals,
collecting D-ray diffraction data, solving the
data set to generate an electron density map, and
interpreting the electron density map.
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Chapter 13. Structure Determination
7
13.3 Mass Spectrometry
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Chapter 13. Structure Determination
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Chapter 13. Structure Determination
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PRACTICE PROBLEM 13.3
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Chapter 13. Structure Determination
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Mass Spectral Fragmentation of Hexane
11
IR Spectrum
12
UV-Vis Spectrum
13
NMR Spectrum
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Electromagnetic spectrum
  • e hu
  • a.IR
  • b.UV
  • c.NMR

15
IR absorption spectrum
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Infrared region
The infrared (IR) region of the electromagnetic
spectrum extends from 7.810-7 m to 10-4 m.   
17
13.2 IR Spectroscopy of Organic Molecules
  • Why does an organic molecule absorb some
    wavelength of IR radiation but not others?
  • a. molecular vibration
  • .stretching
  • .bending
  • b. absorb quantized energy

18
Kinds of allowed Vibrations
  • CH4

19
Information from IR
  • IR spectrum
  • ?
  • What molecular motions?
  • ?
  • What functional groups?

20
Interpreting Infrared Spectra
  • Most functional groups have characteristic IR
    absorption bands that dont change from one
    compound to another.
  • Characteristic IR absorptions of some functional
    groups. (Table 13.1)

21
Table 13-1
22
Infrared spectra of compounds
23
Significant regions of IR
The useful range of IR radiation is 4000 cm-1
400 cm-1 this corresponds to energies of 48.0
kJ/mol 4.8 kJ/mol.
24
13.3 Absorption Spectroscopy
  • The ultraviolet region of interest 200 nm and
    400 nm
  • The energy absorbed is used to promote a p
    electron in a conjugated system from one orbital
    to another.
  • A UV spectrum is a plot of absorbance vs.
    wavelength.
  • UV spectra usually constant of a single broad
    peak, whose maximum is ?max. (Figure13.8 )
  • ?max increase with the degree of conjugation of a
    molecule.  

25
Fig 13.7 The region
26
MO
  • 1,4-butadiene has four ? molecular orbitals
  • HOMO ? LUMO at 217 nm

27
Fig13.8
28
Table 13.2
  • ?max increases as conjugation increases (lower
    energy)

Practice 13.5
29
13.5 NMR Spectroscopy
  • Theory of NMR spectroscopy
  • (1) Many nuclei behave as if they were spinning
    about an axis.
  • The positively charged nuclei produce a magnetic
    field that can interact with an externally
    applied magnetic field (B0).
  • The 13C nucleus and the 1H nucleus behave in
    this manner.
  • In the absence of an external magnetic field the
    spins of magnetic nuclei are randomly oriented.

30
(2) Nuclear spin when a sample containing
these nuclei is placed between the poles of a
strong magnet (B0), the nuclei align themselves
either with the applied field or against the
applied field.
31
(3) The energy difference ?E between nuclear spin
state
The parallel orientation is slightly lower in
energy and is slightly favored.
32
(4) Nuclear magnetic resonance
  • If the sample is irradiation with radio frequency
    (rf) energy of the correct frequency, the nuclei
    of lower energy absorb energy and spin-flip to
    the higher energy state.
  • The frequency of the rf radiation depends on the
    magnetic field strength and on the magnetic
    nuclei.
  • At a magnetic field strength of 2.62T, rf energy
    of 100 MHz is needed to bring a 1H nucleus into
    resonance, and energy of 25 MHz is needed for
    13C.
  • All nuclei with an odd number of protons (1H, 2H,
    19F, 31P) and neutrons (13C) NMR
  • even number of both protons neutrons (12C,
    16O) No NMR

33
schematic operation of an NMR spectrometer
34
13.6 The nature of NMR absorptions
  • (1) Not all 13C nuclei and not all 1H nuclei
    absorb at the same frequency.
  • Each magnetic nucleus is surrounded by electrons
    that set up their own magnetic fields.
  • These little fields oppose the applied field and
    shield the magnetic nuclei
  • BeffectiveBapplied-Blocal
  • These shielded nuclei adsorb at slightly
    different values of magnetic field strength.
  • NMR spectra can be used to map the
    carbon-hydrogen framework of a molecule.

35
(2) NMR spectra
  • The horizontal axis shows effective field
    strength, and the vertical axis shows intensity
    of absorption.
  • Each peak corresponds to a chemically distinct
    nucleus.

36
1H NMR spectrum
37
13C NMR spectrum
38
13.7 Chemical Shifts
  • (1) TMS is used as a reference point
  • The TMS absorption occurs upfield of other
    adsorptions, and is set as the zero point.

39
  • (2) Field strength increases from left
    (downfield) to right (upfield).
  • Nuclei that adsorb downfield require a lower
    field strength for resonance and are deshielded.
  • Nuclei that adsorb upfield require a higher field
    strength and are shielded.

40
  • (3) The chemical shift is the position on the
    chart where a nucleus absorbs.
  • (4) NMR charts are calibrated by using an
    arbitrary scale - the delta scale (ppm).

41
1H NMR spectroscopy
  • (1) Chemical shifts (13.8)
  • Chemical shifts are determined by the local
    magnetic fields surrounding magnetic nuclei.
  • Most 1H NMR chemical shifts are in the range 0
    10d.
  • H (sp3) adsorb at higher field strength.
  • H (sp2) adsorb at lower field strength.
  • Protons on carbons that are bonded to
    electronegative atoms absorb at lower field
    strength.
  • The 1H NMR spectrum can be divided into 5
    regions
  • See Table 13.3

42
(2) Integration of 1H NMR spectra proton
counting (13.9)
  • The area of a peak is proportional to the number
    of protons.
  • To compare two peaks, measure the relative
    heights of the peak areas.

43
(3) Spin-spin splitting (13.10)
  • The tiny magnetic field produced by one nucleus
    can affect the magnetic field felt by other
    nuclei.
  • Protons that have n equivalent neighboring
    protons show a peak in their 1H NMR spectrum that
    is split into n1 smaller peaks (a multiplet).
  • This splitting is caused by the coupling of spins
    of neighboring nuclei.
  • The distance between peaks in a multiplet is
    called the constant (J).

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  • Chemically identical protons dont show spin-spin
    splitting.
  • The signal of a proton with n equivalent
    neighboring protons is split into a multiplet of
    n1 peaks with coupling constant J.
  • Two groups of coupled protons have the same value
    of J.

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13.11 Uses of 1H NMR spectroscopy
1H NMR can be used to identity the products of
reactions.
49
13.12 13C NMR spectroscopy
13C NMR spectroscopy can show the number of
nonequivalent carbons in a molecule and can
identify symmetry in a molecule.
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13.56
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13.57
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13.58
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