lecture7: 123.101

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Unit One Part 7: conformation just when you thought it was safe to look at molecules again... came shape!

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Page 1: Lecture7: 123.101

Unit One Part 7:conformation

just when you thought it was safe to look at molecules

again... came shape!

Page 2: Lecture7: 123.101

strain3D representationsconformations

7Unit OnePart

so very important...but the

lecture that routinely gets the worst feedback

Page 3: Lecture7: 123.101

?what shape are molecules

Page 4: Lecture7: 123.101

?what shape are molecules

we know the shape of each atom...but

what about the molecules...

Page 5: Lecture7: 123.101

what is conformational

isomerism?

Page 6: Lecture7: 123.101

what is conformational

isomerism?

well, first off isomerism is a misnomer! No

isomers here just bond rotation...

Page 7: Lecture7: 123.101

rotationof abond

sorry movies don’t work in the printed

form...

Page 8: Lecture7: 123.101

rotationof abond would have shown this bond

rotating...conformations are different shapes of the same molecule caused by a bond

rotating...no bonds are broken

Page 9: Lecture7: 123.101

representations ofconformationalisomers

H

HH

conventional representation

sawhorseprojection

Newmanprojection

H H

HH H

H

H

H H

H

H H

H

H H

H

H H

H

H H

Page 10: Lecture7: 123.101

representations ofconformationalisomers

H

HH

conventional representation

sawhorseprojection

Newmanprojection

H H

HH H

H

H

H H

H

H H

H

H H

H

H H

H

H H

three common ways of representing these different

conformations but in fairness only the top two are important

to me...

Page 11: Lecture7: 123.101

representations ofconformationalisomers

H

HH

conventional representation

sawhorseprojection

Newmanprojection

H H

HH H

H

H

H H

H

H H

H

H H

H

H H

H

H H

bold line means bond is sticking upwards towards you and the dashed bond is way from you or behind

the page

Page 12: Lecture7: 123.101

representations ofconformationalisomers

H

HH

conventional representation

sawhorseprojection

Newmanprojection

H H

HH H

H

H

H H

H

H H

H

H H

H

H H

H

H H

big circle is the bond...small black

dot is the front atom

Page 13: Lecture7: 123.101

some conformations more favourable... whilst all can

exist...some are more important...

Page 14: Lecture7: 123.101

dihedralangle

H

H H

HH

H

dihedral angle

we’ll start with the simplest

example...ethane

Page 15: Lecture7: 123.101

dihedralangle

H

H H

HH

H

dihedral angle

the dihedral angle (or torsional angle) is defined, in this case, as the angle between a C–H bond on the near carbon and A C–H bond

on the far carbon...

Page 16: Lecture7: 123.101

dihedralangle

H

H H

HH

H

dihedral angle

we are now going to look how the energy of the

molecule changes as we rotate the C–C bond...

Page 17: Lecture7: 123.101

H

HH

H

H H

H

HH

H

H H

H

HH

H

H H

H

HHH

H HH

HHH

H HH

HHH

H H

ener

gy

600 120 180 240 300 360dihedral

angle

H

HH

H

H H

12 kJmol–1

2conformationswe get two extremes...an unstable high energy conformation and a stable low energy conformation

Page 18: Lecture7: 123.101

H

HH

H

H H

H

HH

H

H H

H

HH

H

H H

H

HHH

H HH

HHH

H HH

HHH

H H

ener

gy

600 120 180 240 300 360dihedral

angle

H

HH

H

H H

12 kJmol–1

2conformations

here the H atoms are overlapping...I know it doesn’t look like it (but if I had drawn it like that then you won’t people able to see

the back atoms

Page 19: Lecture7: 123.101

is this picture clearer?

Page 20: Lecture7: 123.101

H

HH

H

H H

H

HH

H

H H

H

HH

H

H H

H

HHH

H HH

HHH

H HH

HHH

H H

ener

gy

600 120 180 240 300 360dihedral

angle

H

HH

H

H H

12 kJmol–1

2conformations

in this conformation the H atoms are as far apart as

the bonds will allow

Page 21: Lecture7: 123.101

you do not needto learn these values!!

Page 22: Lecture7: 123.101

HC

CH

electron cloud repulsion

torsional strain

torsionalstrainthe difference in

energy is caused by electron-electron repulsion (like charges repel opposite attract think of a

magnet). This is called torsional strain

Page 23: Lecture7: 123.101

staggeredconformation

H

HHH

H H

H

H HH

H H H

H HH

HH

Page 24: Lecture7: 123.101

staggeredconformation

H

HHH

H H

H

H HH

H H H

H HH

HH

all these representations show the most stable /

preferred conformation...the staggered conformation...

atoms far apart

Page 25: Lecture7: 123.101

eclipsedconformation

H H

HH H

H

H

H H

H

H H

H

HH

H

H H

Page 26: Lecture7: 123.101

eclipsedconformation

H H

HH H

H

H

H H

H

H H

H

HH

H

H H

all theserepresentations show the least stable / disfavoured

conformation...the eclipsed conformation...atoms as

close as they can get

Page 27: Lecture7: 123.101

H

HH

H

H H

H

HH

H

H H

H

HH

H

H H

H

HHH

H HH

HHH

H HH

HHH

H H

ener

gy

600 120 180 240 300 360dihedral

angle

H

HH

H

H H

12 kJmol–1

2conformations

as the difference is 12 kJmol–1 and three bonds

are overlapping...each bond must contribute...

Page 28: Lecture7: 123.101

torsionalstrain

H

HH

H

H H4kJmol–1

Page 29: Lecture7: 123.101

what about more complex molecules?

Page 30: Lecture7: 123.101

propane

H

HHCH3

H HH

CH3

H H

H HH H

H H H H

H H

staggered

eclipsed

H

HH

H3C

H H

4 kJmol–14 kJmol–1

6 kJmol–1if we add 1 x CH2 and form propane we have the same two conformations

Page 31: Lecture7: 123.101

propane

H

HHCH3

H HH

CH3

H H

H HH H

H H H H

H H

staggered

eclipsed

H

HH

H3C

H H

4 kJmol–14 kJmol–1

6 kJmol–1

eclipsed slightly less favoured as methyl has

more electrons and causes more torsional strain

Page 32: Lecture7: 123.101

CH3CH2...

H

H H

H H

H

CH2CH3

H H

H H1 2

3 4

1 23

4

butaneH

H H H H

H H

H

H H

CH3

CH3

H H

H H

12

3

4

with butane we can rotate three different

C–C bonds...

Page 33: Lecture7: 123.101

CH3CH2...

H

H H

H H

H

CH2CH3

H H

H H1 2

3 4

1 23

4

butaneH

H H H H

H H

H

H H

CH3

CH3

H H

H H

12

3

4

C1–C2 & C3–C4are dull as they are just like propane (2 conformations of

interest)

Page 34: Lecture7: 123.101

C2-C3CH3CH2...

H

H H

H H

H

CH2CH3

H H

H H1 2

3 4

1 23

4

butaneH

H H H H

H H

H

H H

CH3

CH3

H H

H H

12

3

4

but rotation around C2–C3 far more interesting as we now have the relative position of the two methyl groups to

worry about...

Page 35: Lecture7: 123.101

CH3

HH

H3C

H H

H

HCH3

H3C

H H

H

H3CH

H3C

H H

H

HH3CCH3

H H

ener

gy

600 120 180 240 300 360

CH3

HH

H3C

H H

dihedral angle

CH3

HHCH3

H HH

CH3HCH3

H H

now there are four important conformations based on staggered and

eclipsed

Page 36: Lecture7: 123.101

CH3

HH

H3C

H H

H

HCH3

H3C

H H

H

H3CH

H3C

H H

H

HH3CCH3

H H

ener

gy

600 120 180 240 300 360

CH3

HH

H3C

H H

19 kJmol–116 kJmol–1

4 kJmol–1

dihedral angle4conformations

CH3

HHCH3

H HH

CH3HCH3

H H

Page 37: Lecture7: 123.101

©Graham Johnson, Graham Johnson Medical Media, Boulder, Colorado

Noyoudo not

have toremembervalues

Page 38: Lecture7: 123.101

anti-periplanar

no strain

CH3

HH CH3

H3C HH

HH

CH3

H HCH3

H HCH3

H H

staggered

this is the most important

conformation...the most favoured / preferred...

Page 39: Lecture7: 123.101

anti-periplanar

no strain

CH3

HH CH3

H3C HH

HH

CH3

H HCH3

H HCH3

H H

staggered methyl groups (or anyother groups for that matter) are as

far apart as they can be (easiest seen on Newman projection but must get

used to visualising onstick diagram)

Page 40: Lecture7: 123.101

H

H3CH

H3C

H H

CH3

H H

H

H3C H

CH3

HH

H

H3CH

anti-clinaleclipsed

torsional strain16 kJmol–1

torsional strain6 kJmol–1

torsional strain4 kJmol–1

first of the eclipsed but not that important...

Page 41: Lecture7: 123.101

syn-clinal (gauche)staggered

steric strain4 kJmol–1

H

HH3CCH3

H H

CH3

H HH

HH3C

CH3

H HH

H3C H

new kind of staggered conformation...no overlap so no torsional strain...

Page 42: Lecture7: 123.101

steric strain4 kJmol–1

syn-clinal (gauche)staggered

steric strain4 kJmol–1

H

HH3CCH3

H H

CH3

H HH

HH3C

CH3

H HH

H3C H

but two groups are close...and objects don’t like

being close so they repel each other...

Page 43: Lecture7: 123.101

steric strain4 kJmol–1

syn-clinal (gauche)staggered

steric strain4 kJmol–1

H

HH3CCH3

H H

CH3

H HH

HH3C

CH3

H HH

H3C H

...and we get steric strain...basically you can’t have two things occupying

the same space!

Page 44: Lecture7: 123.101

stericstrain

11 kJmol–1

...and these objects really hate it when they eclipse /

overlap...

Page 45: Lecture7: 123.101

CH3

HH

H3C

H H

CH3

H H

CH3

H H

CH3

HH

H3C

HH

syn-periplanareclipsed

torsional & steric strain19 kJmol–1

torsional strain4 kJmol–1

steric strain11 kJmol–1

...so we get the least stable (most disfavoured if that isn’t too many double negatives)

Page 46: Lecture7: 123.101

CH3

HH

H3C

H H

CH3

H H

CH3

H H

CH3

HH

H3C

HH

syn-periplanareclipsed

torsional & steric strain19 kJmol–1

torsional strain4 kJmol–1

steric strain11 kJmol–1

...all bonds overlap (torsional strain) and the two methyl groups

are as close as possible (steric strain)

Page 47: Lecture7: 123.101

Noyoudo not

have toremembervalues

Page 48: Lecture7: 123.101

most importanttwo extremes

CH3

HHCH3

H H

CH3

H3C HH

HH

anti-periplanar

(staggered)

CH3

HH

H3C

H H

CH3

HH

H3C

HH

syn-periplanar

(eclipsed)

learn!

Page 49: Lecture7: 123.101

another important form of strain...

Page 50: Lecture7: 123.101

another important form of strain...

and it has an ace (to my

juvenile mind) name...

Page 51: Lecture7: 123.101

0

20

40

60

80

100

120

3 4 5 6 7 8ring size

ring

stra

in (k

Jmol

–1)

ring strain as we can see, most cyclic systems contain considerable strain...

Page 52: Lecture7: 123.101

0

20

40

60

80

100

120

3 4 5 6 7 8ring size

ring

stra

in (k

Jmol

–1)

ring strain...cyclopropane really

is a very unhappy bunny...but why?

Page 53: Lecture7: 123.101

cyclopropanes

H

HH

C

H

H

H

H

H

H

H

H

H

torsional strain4 kJmol–1

some torsional strain but this only amounts to...24 kJmol–1...the rest comes from...

Page 54: Lecture7: 123.101

ring strain109°

(tetrahedral)

49° 60°90°

19°

108°1°

109°(tetrahedral)

109°(tetrahedral)ring or angle

strain...

Page 55: Lecture7: 123.101

ring strain109°

(tetrahedral)

49° 60°90°

19°

108°1°

109°(tetrahedral)

109°(tetrahedral)

remember an sp3 carbon wants bond angles of 109°...

Page 56: Lecture7: 123.101

ring strain109°

(tetrahedral)

49° 60°90°

19°

108°1°

109°(tetrahedral)

109°(tetrahedral)

...internal angle of atriangle is 60°...so bonds are being bent to accommodate the difference...this causes a

lot of strain!

Page 57: Lecture7: 123.101

H3C NH

O

O

NHN

O HOOH

HH

O

FR–900848

this strain can beharnessed in drugs...and just

for the vets, this is an anti-fungal used to treat infections of the

lung (piccy of a seagulllung)

Page 58: Lecture7: 123.101

and the most important ring...

Page 59: Lecture7: 123.101

and the most important ring...

one you’ll grow to hate by exam time...

Page 60: Lecture7: 123.101

cyclohexane

CC

CCC

C HH

HH

H H

HH

H

H HH

Page 61: Lecture7: 123.101

N O T FLAT

Page 62: Lecture7: 123.101

N O T FLATbenzene is flat

because it has double bonds...

Page 63: Lecture7: 123.101

chair conformation

the chair conformation(as it looks like a recliner apparently) is the most

important and most stable...

Page 64: Lecture7: 123.101

No torsional strain

No angular strain

Page 65: Lecture7: 123.101

H

HH

H

H

HHH

H

H

H

H

H

H

H

H

H

H

H

H

chair conformationthree representations of the same thing...

Page 66: Lecture7: 123.101

H

HH

H

H

HHH

H

H

H

H

H

H

H

H

H

H

H

H

chair conformation

this is the most important...if you like chemistry (or want to do well at it) learn to draw this accurately

Page 67: Lecture7: 123.101

substituents

the substituents on the ring are given special

names depending on their orientation

Page 68: Lecture7: 123.101

RRR

R

R

R

equatorialposition

substituents stick out away from the ring...they are as far from anything as they possibly

can be

Page 69: Lecture7: 123.101

R

RR

R

RR axialpositionthese substituents are

vertical...above and below the ring...they are still quite close

to each other...

Page 70: Lecture7: 123.101

ring ‘flipping’

H

H

H

HH

H

H H

H

H

H

H

HH

H

HHH

H

HH

H

H

H

HH

H

H HH

H

HH HHH

HH

H HH H

H

H

H

H

H

H H

H

H

H

H

H

H

H

H

H

H

H

1 3

5

4

261

1

1

1 1

2

2

3

4

4

5

4

6

6

chair(strain free)

chair(strain free)

boat(strained)

Page 71: Lecture7: 123.101

ring ‘flipping’

H

H

H

HH

H

H H

H

H

H

H

HH

H

HHH

H

HH

H

H

H

HH

H

H HH

H

HH HHH

HH

H HH H

H

H

H

H

H

H H

H

H

H

H

H

H

H

H

H

H

H

1 3

5

4

261

1

1

1 1

2

2

3

4

4

5

4

6

6

chair(strain free)

chair(strain free)

boat(strained)

simply by rotating the bonds we can make the axial substituents

become equatorial (and vice-versa)

Page 72: Lecture7: 123.101

ring ‘flipping’

H

H

H

HH

H

H H

H

H

H

H

HH

H

HHH

H

HH

H

H

H

HH

H

H HH

H

HH HHH

HH

H HH H

H

H

H

H

H

H H

H

H

H

H

H

H

H

H

H

H

H

1 3

5

4

261

1

1

1 1

2

2

3

4

4

5

4

6

6

chair(strain free)

chair(strain free)

boat(strained)

no bonds broken during this...it is just a change

in conformation

Page 73: Lecture7: 123.101

ring ‘flipping’

H

H

H

HH

H

H H

H

H

H

H

HH

H

HHH

H

HH

H

H

H

HH

H

H HH

H

HH HHH

HH

H HH H

H

H

H

H

H

H H

H

H

H

H

H

H

H

H

H

H

H

1 3

5

4

261

1

1

1 1

2

2

3

4

4

5

4

6

6

chair(strain free)

chair(strain free)

boat(strained)

process passes through a nasty, high energy conformation...the

boat...

Page 74: Lecture7: 123.101

ring ‘flipping’

ener

gy

29 kJmol–1

this shows the energy of the molecule during ring flipping...note how the chair is

wonderfully stable and nothing else is...

Page 75: Lecture7: 123.101

boat conformation

disfavoured as the ‘bow’ and ‘stern’ are being

brought close together (steric strain) and...

Page 76: Lecture7: 123.101

boat conformation

H

H

H

HH H

H H

H H

HH

H

H

H

H

H

H

H

H

29 kJmol–1

torsional strain as C–H bonds overlap

Page 77: Lecture7: 123.101

drawingsubstituents

learn todraw the chair

conformation...it will get you marks

in the exam!

Page 78: Lecture7: 123.101

drawhowto

draw a V on an angle and then learn to draw parallel lines

(hmmm, there’s an album title in there somewhere)

Page 79: Lecture7: 123.101

parallellines

draw this one first...same length as before and the

bottom of the new line should be level with the bottom of the

original two lines

Page 80: Lecture7: 123.101

parallellines

second one is parallel and of the same length

Page 81: Lecture7: 123.101

parallelline!

another parallel line (of same length)

Page 82: Lecture7: 123.101

parallelline!another

finally, close the ring with another parallel

line

Page 83: Lecture7: 123.101

carbon skeleton

Page 84: Lecture7: 123.101

?substituentswheredothego

Page 85: Lecture7: 123.101

axialaxial groups are always vertical

Page 86: Lecture7: 123.101

tetrahedralC

carbon is tetrahedral so make the corners look like a tetrahedron

(and this is the bit none of you ever do, it’s bl@@dy frustrating)

Page 87: Lecture7: 123.101

HH

H

top carbons go up

so the three top carbons have a vertical line upwards

NOT down as this would prevent the carbon looking

like a tetrahedron!

Page 88: Lecture7: 123.101

alternate vertical lines

H

HH

H

HH ...and vice-versa for the lower carbons

Page 89: Lecture7: 123.101

equatorialstick outwards (and will be parallel) and guess

what...

Page 90: Lecture7: 123.101

tetrahedralC

carbon is tetrahedral so draw it like that!

Page 91: Lecture7: 123.101

C–Cparallel

to

Page 92: Lecture7: 123.101

parallel linesH

HH

H

H

HHH

H

H

H

H

Page 93: Lecture7: 123.101

and look...a tetrahedral

carbon

H

HH

H

H

HHH

H

H

H

H

Page 94: Lecture7: 123.101

H

HH

H

H

HHH

H

H

H

H more parallel

lines

Page 95: Lecture7: 123.101

H

HH

H

H

HHH

H

H

H

Hand even

more parallel lines

Page 96: Lecture7: 123.101

what happens if we add substituents?

Page 97: Lecture7: 123.101

one substituentCH3

CH3

H

CH3

H

95%equatorial

more stable by8 kJmol–1

5%axial

disfavoured

a single substituent will always go for the

equatorial position...

Page 98: Lecture7: 123.101

one substituentCH3

CH3

H

CH3

H

95%equatorial

more stable by8 kJmol–1

5%axial

disfavoured

remember: ring flipping allows us to change between conformations

without breaking any bonds

Page 99: Lecture7: 123.101

one substituentCH3

CH3

H

CH3

H

95%equatorial

more stable by8 kJmol–1

5%axial

disfavoured

but why equatorial??

Page 100: Lecture7: 123.101

1,3-diaxial interactionsCH3

HHH H

CH3H

H

equatorial position sticks into space...away from ring

Page 101: Lecture7: 123.101

1,3-diaxial interactionsCH3

HHH H

CH3H

H

axial substituent is tucked under ring...and we get interaction between the

three substituents on the same face

Page 102: Lecture7: 123.101

1,3-diaxial interactionsCH3

HHH H

CH3H

Hknown as 1,3-diaxial

interaction

Page 103: Lecture7: 123.101

H

H

equatorialfavoured

axialdisfavoured

one big substituent

X

when you have a big substituent it fixes the

ring and stop ring flip...

Page 104: Lecture7: 123.101

HH

H

HHH

1,3-diaxial interactions

Page 105: Lecture7: 123.101

HH

H

HHH

1,3-diaxial interactions

...because 1,3-diaxial interaction really

disfavoured

Page 106: Lecture7: 123.101

•conformations of molecules

•conformations of cyclohexane

what have....we learnt?

Picture: © Chris Ewels

Page 107: Lecture7: 123.101

©Pink Sherbet Photography@flickr

practice drawing thecyclohexane chair

Page 108: Lecture7: 123.101

©Pragmagraphr@flickr

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