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1 Chapter 9 Nuclear Magnetic Resonance and Mass Spectrometry About The Authors These PowerPoint Lecture Slides were created and prepared by Professor William Tam and his wife Dr Phillis Chang ID: 273602

signal nmr shift chemical nmr signal chemical shift spectrum peak protons number carbon atoms molecular ppm hydrogen proton hydrogens

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Slide1

Ch. 9 - 1

Chapter 9

Nuclear Magnetic

Resonance and Mass

SpectrometrySlide2

About The Authors

These PowerPoint Lecture Slides were created and prepared by Professor William Tam and his wife Dr. Phillis Chang.

Professor William Tam received his B.Sc. at the University of Hong Kong in 1990 and his Ph.D. at the University of Toronto (Canada) in 1995. He was an NSERC postdoctoral fellow at the Imperial College (UK) and at Harvard University (USA). He joined the Department of Chemistry at the University of Guelph (Ontario, Canada) in 1998 and is currently a Full Professor and Associate Chair in the department. Professor Tam has received several awards in research and teaching, and according to

Essential Science Indicators, he is currently ranked as the Top 1% most cited Chemists worldwide. He has published four books and over 80 scientific papers in top international journals such as J. Am. Chem. Soc., Angew. Chem., Org. Lett., and J. Org. Chem. Dr. Phillis Chang received her B.Sc. at New York University (USA) in 1994, her M.Sc. and Ph.D. in 1997 and 2001 at the University of Guelph (Canada). She lives in Guelph with her husband, William, and their son, Matthew.

Ch. 9 -

2Slide3

Ch. 9 - 3

Introduction

Classic methods for organic structure determination

Boiling point

Refractive index

Solubility tests

Functional group tests

Derivative preparation

Sodium fusion (to identify N, Cl, Br, I & S)

Mixture melting point

Combustion analysis

DegradationSlide4

Ch. 9 - 4

Classic methods for organic structure determination

Require large quantities of sample and are time consumingSlide5

Ch. 9 - 5

Spectroscopic methods for organic structure determination

Mass Spectroscopy (MS)

Molecular Mass & characteristic fragmentation

patternInfrared Spectroscopy (IR)Characteristic functional groups

Ultraviolet Spectroscopy (UV)

Characteristic chromophore

Nuclear Magnetic Resonance (NMR)Slide6

Ch. 9 - 6

Spectroscopic methods for organic structure determination

Combination of these spectroscopic techniques provides a rapid, accurate and powerful tool for Identification and Structure Elucidation of organic compounds

Rapid

Effective in mg and microgram quantitiesSlide7

Ch. 9 - 7

General steps for structure elucidation

Elemental analysis

Empirical formula

e.g. C2H4OMass spectroscopy

Molecular weight

Molecular formula

e.g. C

4

H

8

O

2

, C

6

H

12

O

3

… etc.

Characteristic fragmentation pattern for certain functional groupsSlide8

Ch. 9 - 8

General steps for structure elucidation

From molecular formula

Double bond equivalent (DBE)

Infrared spectroscopy (IR)Identify some specific functional groups

e.g. C=O, C–O, O–H, COOH, NH

2

… etc.Slide9

Ch. 9 - 9

General steps for structure elucidation

UV

Sometimes useful especially for conjugated systems

e.g. dienes, aromatics, enones1H, 13

C NMR and other advanced NMR techniques

Full structure determination Slide10

Ch. 9 - 10

Electromagnetic spectrumSlide11

Ch. 9 - 11

Nuclear Magnetic Resonance

(NMR) Spectroscopy

A graph that shows the characteristic energy absorption frequencies and intensities for a sample in a magnetic field is called a

nuclear magnetic resonance (NMR) spectrumSlide12

Ch. 9 - 12Slide13

Ch. 9 - 13

The number of signals in the spectrum tells us how many different sets of protons there are in the molecule

The position of the signals in the spectrum along the x-axis tells us about the magnetic environment of each set of protons arising largely from the electron density in their environmentSlide14

Ch. 9 - 14

The area under the signal tells us about how many protons there are in the set being measured

The multiplicity (or splitting pattern) of each signal tells us about the number of protons on atoms adjacent to the one whose signal is being measuredSlide15

Ch. 9 - 15

Typical

1

H NMR spectrum

Chemical Shift ()Integration (areas of peaks

no. of H)

Multiplicity (spin-spin splitting) and coupling constantSlide16

Ch. 9 - 16

Typical

1

H NMR spectrumSlide17

Ch. 9 - 17

2A.

Chemical Shift

The position of a signal along the

x

-axis of an NMR spectrum is called its

chemical shift

The chemical shift of each signal gives information about the structural environment of the nuclei producing that signal

Counting the number of signals in a

1

H NMR spectrum indicates, at a first approximation, the number of distinct proton environments in a moleculeSlide18

Ch. 9 - 18Slide19

Ch. 9 - 19Slide20

Ch. 9 - 20

Normal range of

1

H NMRSlide21

Ch. 9 - 21

Reference compound

TMS = tetramethylsilane

as a reference standard (0 ppm)

Reasons for the choice of TMS as reference

Resonance position at higher field than other organic compounds

Unreactive and stable, not toxic

Volatile and easily removed

(B.P. = 28

o

C)Slide22

Ch. 9 - 22

NMR solvent

Normal NMR solvents should not contain hydrogen

Common solvents

CDCl3

C

6

D

6

CD

3

OD

CD

3

COCD

3

(d

6

-acetone)Slide23

Ch. 9 - 23

The 300-MHz

1

H NMR spectrum of 1,4-dimethylbenzeneSlide24

Ch. 9 - 24

2B.

Integration of Signal

Areas

Integral

Step

Heights

The area under each signal in a

1

H NMR spectrum is proportional to the number of hydrogen atoms producing that signal

It is signal area (integration), not signal height, that gives information about the number of hydrogen atomsSlide25

Ch. 9 - 25

H

a

H

b

2 H

a

3 H

bSlide26

Ch. 9 - 26

2C.

Coupling (Signal Splitting)

Coupling is caused by the magnetic effect of nonequivalent hydrogen atoms that are within 2 or 3 bonds of the hydrogens producing the signal

The

n

+1 rule

Rule of Multiplicity:

If a proton (or a set of magnetically equivalent nuclei) has

n

neighbors of magnetically equivalent protons. It’s multiplicity is

n

+ 1Slide27

Ch. 9 - 27

ExamplesSlide28

Ch. 9 - 28Slide29

Ch. 9 - 29

Examples

Note: All

H

b’s are chemically and magnetically equivalent.Slide30

Ch. 9 - 30

Pascal’s Triangle

Use to predict relative intensity of various peaks in multiplet

Given by the coefficient of binomial expansion (a + b)

nsinglet (s) 1

doublet (d) 1 1

triplet (t) 1 2 1

quartet (q) 1 3 3 1

quintet 1 4 6 4 1

sextet 1 5 10 10 5 1Slide31

Ch. 9 - 31

Pascal’s Triangle

For

For

Due to symmetry,

H

a

and

H

b

are identical

a singlet

H

a

H

b

two doubletsSlide32

Ch. 9 - 32

How to Interpret Proton NMR

Spectra

Count the number of signals to determine how many distinct proton environments are in the molecule (neglecting, for the time being, the possibility of overlapping signals)

Use chemical shift tables or charts to correlate chemical shifts with possible structural environmentsSlide33

Ch. 9 - 33

Determine the relative area of each signal, as compared with the area of other signals, as an indication of the relative number of protons producing the signal

Interpret the splitting pattern for each signal to determine how many hydrogen atoms are present on carbon atoms adjacent to those producing the signal and sketch possible molecular fragments

Join the fragments to make a molecule in a fashion that is consistent with the dataSlide34

Ch. 9 - 34

Example:

1

H NMR (300 MHz) of an unknown compound with molecular formula C

3H7BrSlide35

Ch. 9 - 35

Three distinct signals at

~

d

3.4, 1.8 and 1.1

ppm

d

3.4

ppm: likely to be near an

electronegative

group (Br)Slide36

Ch. 9 - 36

d

(ppm):

3.4

1.8 1.1

Integral:

2

2

3Slide37

Ch. 9 - 37

d

(ppm):

3.4

1.8 1.1

Multiplicity:

triplet

sextet

triplet

2 H

'

s on adjacent C

5 H

'

s on adjacent C

2 H

'

s on adjacent CSlide38

Ch. 9 - 38

Complete structure:

2 H

'

s from integration

triplet

2 H

'

s from integration

sextet

3 H

'

s from integration

triplet

most upfield signal

most downfield

signalSlide39

Ch. 9 - 39

Nuclear Spin:

The Origin of the Signal

The magnetic field associated with a spinning proton

The spinning proton resembles a tiny bar magnetSlide40

Ch. 9 - 40Slide41

Ch. 9 - 41Slide42

Ch. 9 - 42

Spin quantum number (I)

1

H: I =

½ (two spin states: +½ or -½)

(similar for

13

C,

19

F,

31

P)

12

C,

16

O,

32

S: I = 0

 These nuclei do not give an NMR spectrumSlide43

Ch. 9 - 43

Detecting the Signal: Fourier

Transform NMR SpectrometersSlide44

Ch. 9 - 44Slide45

Ch. 9 - 45

All protons do not absorb energy at the same frequency in a given external magnetic field

Lower chemical shift values correspond with lower frequency

Higher chemical shift values correspond with higher frequency

Shielding & Deshielding of ProtonsSlide46

Ch. 9 - 46Slide47

Ch. 9 - 47

Deshielding by electronegative groups

CH

3

X

X =

F

OH

Cl

Br

I

H

Electro-negativity

4.0

3.5

3.1

2.8

2.5

2.1

d

(ppm)

4.26

3.40

3.05

2.68

2.16

0.23

Greater electronegativity

Deshielding of the proton

Larger

dSlide48

Ch. 9 - 48

Shielding and deshielding by circulation of

p

electrons

If we were to consider only the relative electronegativities of carbon in its three hybridization states, we might expect the following order of protons attached to each type of carbon:(higher frequency)

sp < sp

2

< sp

3

(lower frequency)Slide49

Ch. 9 - 49

In fact, protons of terminal alkynes absorb between

d

2.0 and

d 3.0, and the order is(higher frequency)

sp

2

< sp < sp

3

(lower frequency)Slide50

Ch. 9 - 50

This upfield shift (lower frequency) of the absorption of protons of terminal alkynes is a result of shielding produced by the circulating

p

electrons of the triple bond

Shielded

(

d

2 – 3 ppm)Slide51

Ch. 9 - 51

Aromatic system

Shielded region

Deshielded regionSlide52

Ch. 9 - 52

e.g.

d

(ppm)

Ha

& H

b

: 7.9 & 7.4 (deshielded)

H

c

& H

d

: 0.91 – 1.2 (shielded)Slide53

Ch. 9 - 53

Alkenes

Deshielded

(

d

4.5 – 7 ppm)Slide54

Ch. 9 - 54

Aldehydes

Electronegativity effect + Anisotropy effect

d

= 8.5 – 10 ppm (deshielded)Slide55

Ch. 9 - 55

Reference compound

TMS = tetramethylsilane

as a reference standard (0 ppm)

Reasons for the choice of TMS as referenceResonance position at higher field than other organic compounds

Unreactive and stable, not toxic

Volatile and easily removed

(B.P. = 28

o

C)

The Chemical ShiftSlide56

Ch. 9 - 56

7A.

PPM and the

d

Scale

The chemical shift of a proton, when expressed in

hertz (Hz)

, is proportional to the strength of the external magnetic field

Since spectrometers with different magnetic field strengths are commonly used, it is desirable to express chemical shifts in a form that is independent of the strength of the external fieldSlide57

Ch. 9 - 57

Since chemical shifts are always very small (typically 5000 Hz) compared with the total field strength (commonly the equivalent of 60, 300, or 600

million

hertz), it is convenient to express these fractions in units of

parts per million (ppm)This is the origin of the delta scale for the expression of chemical shifts relative to TMSSlide58

Ch. 9 - 58

For example, the chemical shift for benzene protons is 2181 Hz when the instrument is operating at 300 MHz. Therefore

The chemical shift of benzene protons in a 60 MHz instrument is 436 Hz:

Thus, the chemical shift expressed in ppm is the same whether measured with an instrument operating at 300 or 60 MHz (or any other field strength)Slide59

Ch. 9 - 59

Two or more protons that are in identical environments have the same chemical shift and, therefore, give only one

1

H NMR signal

Chemically equivalent protons are chemical shift equivalent in 1H NMR spectra

Chemical Shift Equivalent and

Nonequivalent ProtonsSlide60

Ch. 9 - 60

8A.

Homotopic and Heterotopic Atoms

If replacing the hydrogens by a different atom gives the same compound, the hydrogens are said to be

homotopic

Homotopic hydrogens have identical environments and will have the same chemical shift. They are said to be

chemical shift equivalentSlide61

Ch. 9 - 61

The six hydrogens of ethane are

homotopic

and are, therefore,

chemical shift equivalent

Ethane, consequently, gives only one signal in its

1

H NMR spectrum

same compounds

same compoundsSlide62

Ch. 9 - 62

If replacing hydrogens by a different atom gives

different compounds

, the hydrogens are said to be

heterotopicHeterotopic atoms have different chemical shifts and are not chemical shift equivalentSlide63

Ch. 9 - 63

These 2 H’s are also

homotopic

to each other

different compounds

heterotopic

same compounds

 these 3 H’s of the CH

3

group are

homotopic

 the CH

3

group gives only one 1H NMR signalSlide64

Ch. 9 - 64

CH

3

CH

2

Br

two sets of hydrogens that are heterotopic with respect to each other

two

1

H NMR signalsSlide65

Ch. 9 - 65

Other examples

 2

1

H NMR signals

 4

1

H NMR signalsSlide66

Ch. 9 - 66

Other examples

 3

1

H NMR signalsSlide67

Ch. 9 - 67

Application to

13

C NMR spectroscopy

Examples

 1

13

C NMR signal

 4

13

C NMR signalsSlide68

Ch. 9 - 68

 5

13

C NMR signals

 4

13

C NMR signalsSlide69

Ch. 9 - 69

8B.

Enantiotopic and Diastereotopic

Hydrogen Atoms

If replacement of each of two hydrogen atoms by the same group yields compounds that are enantiomers, the two hydrogen atoms are said to be

enantiotopicSlide70

Ch. 9 - 70

Enantiotopic hydrogen atoms have the same chemical shift and give only one

1

H NMR signal:

enantiomer

enantiotopicSlide71

Ch. 9 - 71

diastereomers

diastereotopic

chirality

centreSlide72

Ch. 9 - 72

diastereomers

diastereotopicSlide73

Ch. 9 - 73

Vicinal coupling

is coupling between hydrogen atoms on adjacent carbons (vicinal hydrogens), where separation between the hydrogens is by three

s

bondsSignal Splitting:Spin–Spin CouplingSlide74

Ch. 9 - 74

9A.

Vicinal Coupling

Vicinal coupling between heterotopic protons generally follows the

n

+ 1 rule. Exceptions to the

n

+ 1 rule can occur when diastereotopic hydrogens or conformationally restricted systems are involved

Signal splitting is not observed for protons that are homotopic (chemical shift equivalent) or enantiotopicSlide75

Ch. 9 - 75

9B.

Splitting Tree Diagrams and the

Origin of Signal Splitting

Splitting analysis for a doubletSlide76

Ch. 9 - 76

Splitting analysis for a tripletSlide77

Ch. 9 - 77

Splitting analysis for a quartetSlide78

Ch. 9 - 78

Pascal’s Triangle

Use to predict relative intensity of various peaks in multiplet

Given by the coefficient of binomial expansion (a + b)

nsinglet (s) 1

doublet (d) 1 1

triplet (t) 1 2 1

quartet (q) 1 3 3 1

quintet 1 4 6 4 1

sextet 1 5 10 10 5 1Slide79

Ch. 9 - 79

9C.

Coupling Constants

Recognizing

Splitting PatternsSlide80

Ch. 9 - 80

9D.

The Dependence of Coupling

Constants on Dihedral Angle

3

J values are related to the dihedral angle (

)Slide81

Ch. 9 - 81

Karplus curve

f

~0

o or 180o

Maximum

3

J value

f

~90

o

3

J ~0 HzSlide82

Ch. 9 - 82

Karplus curve

ExamplesSlide83

Ch. 9 - 83

Karplus curve

ExamplesSlide84

Ch. 9 - 84

9E.

Complicating Features

The 60 MHz

1

H NMR spectrum of ethyl chloroacetateSlide85

Ch. 9 - 85

The 300 MHz

1

H NMR spectrum of ethyl chloroacetateSlide86

Ch. 9 - 86

9F.

Analysis of Complex InteractionsSlide87

Ch. 9 - 87

The 300 MHz

1

H NMR spectrum of 1-nitropropaneSlide88

Ch. 9 - 88

Protons of alcohols (ROH) and amines may appear over a wide range from 0.5 – 5.0 ppm

Hydrogen-bonding is the reason for this range

Proton NMR Spectra and Rate

ProcessesSlide89

Ch. 9 - 89

Why don’t we see coupling with the O–H proton, e.g. –CH

2

–OH (triplet?)

Because the acidic protons are exchangeable about 105 protons per second (residence time 10-5 sec), but the NMR experiment requires a time of 10-2 – 10-3 sec. to “take” a spectrum, usually we just see an average (thus, OH protons are usually a broad singlet) Slide90

Ch. 9 - 90

Trick:

Run NMR in d

6

-DMSO where H-bonding with DMSO’s oxygen prevents H’s from exchanging and we may be able to see the coupling Slide91

Ch. 9 - 91

Deuterium Exchange

To determine which signal in the NMR spectrum is the OH proton, shake the NMR sample with a drop of D

2

O and whichever peak disappears that is the OH peak (note: a new peak of HOD appears)Slide92

Ch. 9 - 92

Phenols

Phenol protons appear downfield at 4-7 ppm

They are more “acidic” - more H+ character More dilute solutions - peak appears upfield: towards 4 ppm Slide93

Ch. 9 - 93

Phenols

Intramolecular H-bonding causes downfield shift

12.1 ppmSlide94

Ch. 9 - 94

Unlike

1

H with natural abundance ~99.98%, only 1.1% of carbon, namely

13C, is NMR activeCarbon-13 NMR Spectroscopy

11A.

Interpretation of

13

C NMR

SpectraSlide95

Ch. 9 - 95

11B.

One Peak for Each Magnetically

Distinct Carbon Atom

13

C NMR spectra have only become commonplace more recently with the introduction of the Fourier Transform (FT) technique, where averaging of many scans is possible (note

13

C spectra are 6000 times weaker than

1

H spectra, thus require a lot more scans for a good spectrum)Slide96

Ch. 9 - 96

Note for a 200 MHz NMR (field strength 4.70 Tesla)

1

H NMR

 Frequency = 200 MHz

13

C NMR

Frequency = 50 MHzSlide97

Ch. 9 - 97

Example:

2-Butanol

Proton-coupled

13

C NMR spectrumSlide98

Ch. 9 - 98

Example:

2-Butanol

Proton-decoupled

13

C NMR spectrumSlide99

Ch. 9 - 99

11C.

13

C Chemical Shifts

Decreased electron density around an atom

deshields

the atom from the magnetic field and causes its signal to occur further

downfield

(higher ppm, to the left) in the NMR spectrum

Relatively higher electron density around an atom

shields

the atom from the magnetic field and causes the signal to occur

upfield

(lower ppm, to the right) in the NMR spectrumSlide100

Ch. 9 - 100

Factors affecting chemical shift

Diamagnetic shielding due to bonding electrons

Paramagnetic shielding due to low-lying electronic excited state Magnetic Anisotropy – through space due to the near-by group (especially

electrons)

In

1

H NMR, (i) and (iii) most significant; in

13

C NMR, (ii) most significant (since chemical shift range >>

1

H NMR) Slide101

Ch. 9 - 101

Electronegative substituents cause downfield shift

Increase in relative atomic mass of substituent

causes upfield shiftSlide102

Ch. 9 - 102

Hybridization of carbon

sp

2

> sp > sp

3

123.3 ppm

71.9 ppm

5.7 ppmSlide103

Ch. 9 - 103

Anisotropy effect

Shows shifts similar to the effect in

1

H NMR

shows large

upfield shiftSlide104

Ch. 9 - 104Slide105

Ch. 9 - 105Slide106

Ch. 9 - 106

(a)

(b)

(c)Slide107

Ch. 9 - 107

11D.

Off-Resonance Decoupled Spectra

NMR spectrometers can differentiate among carbon atoms on the basis of the number of hydrogen atoms that are attached to each carbon

In an off-resonance decoupled

13

C NMR spectrum, each carbon signal is split into a multiplet of peaks, depending on how many hydrogens are attached to that carbon. An

n

+ 1 rule applies, where

n

is the number of hydrogens on the carbon in question. Thus, a carbon with no hydrogens produces a singlet (

n

= 0), a carbon with one hydrogen produces a doublet (two peaks), a carbon with two hydrogens produces a triplet (three peaks), and a methyl group carbon produces a quartet (four peaks)Slide108

Ch. 9 - 108

Off-resonance decoupled

13

C NMR

Broadband proton-decoupled

13

C NMRSlide109

Ch. 9 - 109

11E.

DEPT

13

C Spectra

DEPT

13

C NMR spectra

indicate how many hydrogen atoms are bonded to each carbon, while also providing the chemical shift information contained in a broadband proton-decoupled

13

C NMR spectrum. The carbon signals in a DEPT spectrum are classified as CH

3

, CH

2

, CH, or C accordinglySlide110

Ch. 9 - 110

(a)

(b)

(c)Slide111

Ch. 9 - 111

The broadband proton-decoupled

13

C NMR spectrum of methyl methacrylateSlide112

Ch. 9 - 112

HCOSY

1

H–

1H correlation spectroscopyHETCOR

Heteronuclear correlation spectroscopy

Two-Dimensional (2D) NMR

TechniquesSlide113

Ch. 9 - 113

HCOSY of 2-chloro-butane

H

2

H

1

H

1

H

3

H

3

H

4

H

4

H

2Slide114

Ch. 9 - 114

HETCOR

of 2-chloro-butane

H

1

H

2

H

3

H

4

C

1

C

2

C

3

C

4Slide115

Ch. 9 - 115

Partial MS of octane (C

8

H

18, M = 114)An Introduction to Mass

SpectrometrySlide116

Ch. 9 - 116

The M

+

peak at 114 is referred to as the

parent peak or molecular ion

The largest or most abundant peak is called the

base peak

and is assigned an intensity of 100%, other peaks are then fractions of that e.g. 114(M

+

,40), 85(80), 71(60), 57(100) etc. Slide117

Ch. 9 - 117

Masses are usually rounded off to whole numbers assuming:

H = 1, C = 12, N = 14, O = 16, F = 19 etc.

Molecular ion (parent peak)

Daughter

ionsSlide118

Ch. 9 - 118

In the mass spectrometer, a molecule in the gaseous phase under low pressure is bombarded with a beam of high-energy electrons (70 eV or ~ 1600 kcal/mol)

This beam can dislodge an electron from a molecule to give a radical cation which is called the molecular ion, M

+ or more accurately

Formation of Ions: Electron

Impact IonizationSlide119

Ch. 9 - 119

This molecular ion has considerable surplus energy so it can fly apart or fragment to give specific ions which may be diagnostic for a particular compoundSlide120

Ch. 9 - 120

Depicting the Molecular Ion

Radical cations from ionization

of nonbonding on

p

electronSlide121

Ch. 9 - 121

Compound

Ionization

Potential (eV)

CH

3

(CH

2

)

3

NH

2

8.7

C

6

H

6

(benzene)

9.2

C

2

H

4

10.5

CH

3

OH

10.8

C

2

H

6

11.5

CH

4

12.7

Ionization potentials of selected moleculesSlide122

Ch. 9 - 122

Fragmentation

The reactions that take place in a mass spectrometer are unimolecular, that is, they do not involve collisions between molecules or ions. This is true because the pressure is kept so low (10

-6

torr) that reactions involving bimolecular collisions do not occur

We use single-barbed arrows to depict mechanisms involving single electron movements

The relative ion abundances, as indicated by peak intensities, are very importantSlide123

Ch. 9 - 123

16A.

Fragmentation by Cleavage at a

Single Bond

When a molecular ion fragments, it will yield a neutral radical (not detected) and a carbocation (detected) with an even number of electrons

The fragmentation will be dictated to some extent by the fragmention of the more stable carbocation:

ArCH

2

+

> CH

2

=CHCH

2

+

> 3

o

> 2

o

> 1

o

> CH

3

+

Slide124

Ch. 9 - 124

e.g.

X

Site of ionization:

n >

p

>

s

non-bondingSlide125

Ch. 9 - 125

As the carbon skeleton becomes more highly branched, the intensity of the molecular ion peak decreases

Butane vs. isobutane

a

bSlide126

Ch. 9 - 126

16B.

Fragmentation of Longer Chain

and Branched Alkanes

Octane vs. isooctaneSlide127

Ch. 9 - 127

16C.

Fragmentation to Form

Resonance-Stabilized Cations

Alkenes

Important fragmentation of terminal alkenes

Allyl carbocation (m/e = 41) Slide128

Ch. 9 - 128

Carbon–carbon bonds next to an atom with an unshared electron pair usually break readily because the resulting carbocation is resonance stabilized

Ethers

Cleavage

a (to ether oxygen) C–C bondsSlide129

Ch. 9 - 129

Alcohols

Most common fragmentation: - loss of alkyl groups

a

bSlide130

Ch. 9 - 130

Carbon–carbon bonds next to the carbonyl group of an aldehyde or ketone break readily because resonance-stabilized ions called

acylium ions

are producedSlide131

Ch. 9 - 131

Aldehydes

M

+

peak usually observed but may be fairly weakCommon fragmentation patterna

-cleavageSlide132

Ch. 9 - 132

Ketones

a

-cleavage

a

a

b

bSlide133

Ch. 9 - 133

Alkyl-substituted benzenes ionize by loss of a

π

electron and undergo loss of a hydrogen atom or methyl group to yield the relatively stable tropylium ion (see Section 14.7C). This fragmentation gives a prominent peak (sometimes the base peak) at

m/z 91Slide134

Ch. 9 - 134

Aromatic hydrocarbons

very intense M

+

peaks characteristic fragmentation pattern (when an alkyl group attached to the benzene ring): - tropylium cation Slide135

Ch. 9 - 135

16D.

Fragmentation by Cleavage of

Two Bonds

Alcohols frequently show a prominent peak at M

- 18. This corresponds to the loss of a molecule of water

May lose H

2

O by 1,2- or 1,4-eliminationSlide136

Ch. 9 - 136Slide137

Ch. 9 - 137

Cycloalkenes show a characteristic fragmentation pattern which corresponds to a reverse Diels-Alder reaction

e.g.Slide138

Ch. 9 - 138

Aromatic hydrocarbons

e.g.Slide139

Ch. 9 - 139

Ketones

McLafferty rearrangement Slide140

Ch. 9 - 140Slide141

Ch. 9 - 141

Characteristic of McLafferty rearrangement

No alkyl migrations to C=O, only H migrates

XSlide142

Ch. 9 - 142

Characteristic of McLafferty rearrangement

2

o

is preferred over 1oSlide143

Ch. 9 - 143

How To Determine Molecular

Formulas and Molecular Weights

Using Mass Spectrometry

17A.

Isotopic Peaks & the Molecular IonSlide144

Ch. 9 - 144

The presence of isotopes of carbon, hydrogen, and nitrogen in a compound gives rise to a small M + 1 peak

The presence of oxygen, sulfur, chlorine, or bromine in a compound gives rise to an

M +

2 peakSlide145

Ch. 9 - 145

The M + 1 peak can be used to determine the number of carbons in a molecule

The

M +

2 peak can indicate whether bromine or chlorine is presentThe isotopic peaks, in general, give us one method for determining molecular formulasSlide146

Ch. 9 - 146

Example

Consider 100 molecules of CH

4

C12: 100 C

13

: 1.11

H

1

: 100 H

2

: 0.016Slide147

Ch. 9 - 147

1.11 molecules contain a

13

C atom

4x0.016 = 0.064 molecules contain a

2

H atom

Intensity of

M

+ 1 peak:

1.11+0.064=1.174% of the

M

peakSlide148

Ch. 9 - 148

100

1.17

m

/z

relative ion abundance

M

M +1Slide149

Ch. 9 - 149

17B.

How To

Determine

the Molecular

Formula

m/z

Intensity

(% of

M

)

72

73.0/73 x 100 = 100

73

3.3/73 x 100 = 4.5

74

0.2/73 x 100 = 0.3Slide150

Ch. 9 - 150

Is M odd or even? According to the nitrogen rule

,

if it is even, then the compound must contain an even number of nitrogen atoms (zero is an even number)

For our unknown, M is even. The compound must have an even number of nitrogen atomsSlide151

Ch. 9 - 151

The relative abundance of the M +1 peak indicates the number of carbon atoms. Number of C atoms =

relative abundance of (M +1)/1.1

For our unknownSlide152

Ch. 9 - 152

The relative abundance of the M +2 peak indicates the presence (or absence) of S (4.4%), Cl (33%), or Br (98%)

For our unknown M +2 = 0.3%; thus, we can assume that S, Cl, and Br are absent

The molecular formula can now be established by determining the number of hydrogen atoms and adding the appropriate number of oxygen atoms, if necessarySlide153

Ch. 9 - 153

Since M is m

/z 72

 molecular weight = 72

As determined using the relative abundance of M +1 peak, number of carbons present is 4Using the “nitrogen rule”, this unknown must have an even number of N. Since M.W. = 72, and there are 4 C present, (12 x 4 = 48), adding 2 “N” will be greater than the M.W. of the unknown. Thus, this unknown contains zero “N”Slide154

Ch. 9 - 154

For a molecule composed of C and H only

H = 72 – (4 x 12) = 24

but C4H24

is impossible

For a molecule composed of C, H and O

H = 72 – (4 x 12) – 16 = 8

and thus our unknown has the molecular formula C

4

H

8

OSlide155

Ch. 9 - 155

17C.

High-Resolution Mass SpectrometrySlide156

Ch. 9 - 156

Example 1

O

2

, N2H4 and CH3OH all have M.W. of 32 (by MS), but accurate masses are differentO2 = 2(15.9949) = 31.9898

N

2

H

4

= 2(14.0031) + 4(1.00783) = 32.0375

CH

4

O = 12.00000 + 4(1.00783) + 15.9949 = 32.0262Slide157

Ch. 9 - 157

Example 2

Both C

3

H8O and C2H4O2 have M.W. of 60 (by MS), but accurate masses are different

C

3

H

8

O = 60.05754

C

2

H

4

O

2

= 60.02112Slide158

Ch. 9 - 158

Mass Spectrometer Instrument

DesignsSlide159

Ch. 9 - 159

19. GC/MS AnalysisSlide160

Ch. 9 - 160

 END OF CHAPTER 9 

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