Infrared Spectroscopy
A concise revision guide to infrared spectroscopy: why bonds absorb infrared radiation, wavenumbers and transmittance, the characteristic absorptions of C–H, C=C, C=O, O–H, N–H and C–X bonds, the fingerprint region, and the link to greenhouse gases.
- 4.2.4(a)
- 4.2.4(b)-i
- 4.2.4(b)-ii
- 4.2.4(c)(i)
- 4.2.4(c)(ii)
- 4.2.4(c)(iii)
- 4.2.4(d)-i
- 4.2.4(d)-ii
- 4.2.4(e)-i
- 4.2.4(e)-ii
What these spec points say
- 4.2.4(a) infrared (IR) radiation causes covalent bonds to vibrate more and absorb energy
- 4.2.4(b)-i absorption of infrared radiation by atmospheric gases containing C=O, O–H and C–H bonds (e.g. CO2, H2O and CH4)
- 4.2.4(b)-ii the suspected link between absorption of infrared radiation by atmospheric gases and global warming
- 4.2.4(c)(i) use of an infrared spectrum of an organic compound to identify an alcohol from an absorption peak of the O–H bond
- 4.2.4(c)(ii) use of an infrared spectrum of an organic compound to identify an aldehyde or ketone from an absorption peak of the C=O bond
- 4.2.4(c)(iii) use of an infrared spectrum of an organic compound to identify a carboxylic acid from an absorption peak of the C=O bond and a broad absorption peak of the O–H bond
- 4.2.4(d)-i interpretations of an infrared spectrum of familiar or unfamiliar substances using supplied data
- 4.2.4(d)-ii predictions of an infrared spectrum of familiar or unfamiliar substances using supplied data
- 4.2.4(e)-i use of infrared spectroscopy to monitor gases causing air pollution (e.g. CO and NO from car emissions)
- 4.2.4(e)-ii use of infrared spectroscopy in modern breathalysers to measure ethanol in the breath
Infrared Spectroscopy: Bonds that Absorb
Watch infrared radiation set the bonds of ethanol vibrating, see each bond draw its own trough in the spectrum, then tell an aldehyde and a carboxylic acid apart and see why CO₂ and water vapour are greenhouse gases.
© Dr. Mohammed Al-Fatah – onlinelearningsystem.net
GCSE Recap: Bonds and Energy
Three quick questions on covalent bonds, the electromagnetic spectrum and why greenhouse gases warm the atmosphere.
Why Bonds Absorb Infrared
The atoms joined by a covalent bond are always vibrating: the bond stretches and compresses, and the angles between bonds bend.
Each vibration has its own natural frequency, which depends on the masses of the atoms and the strength of the bond.
When infrared radiation of that same frequency passes through the sample, the bond absorbs it and vibrates more energetically. An infrared spectrometer records which frequencies are absorbed, so the spectrum shows which bonds are present.
The frequency is given as a wavenumber in cm⁻¹ (the number of waves per centimetre), plotted from about 4000 on the left to 500 on the right.
The y-axis is transmittance, the percentage of the radiation that passes through, so an absorption appears as a trough pointing downwards.
Stronger bonds and lighter atoms vibrate faster and absorb at higher wavenumbers: O–H and N–H absorb near 3300 cm⁻¹, C=O near 1700 cm⁻¹, and C–Cl near 700 cm⁻¹.
Key idea: A bond absorbs infrared radiation at the frequency of its own vibration. The wavenumber of the trough identifies the bond.
Characteristic Absorptions
The region above 1500 cm⁻¹ is used for functional group identification, because the absorptions there belong to particular bonds and are listed in the OCR data sheet.
The exam provides the table; the skill is to match each trough to a bond and to give the range in the answer.
| Bond | Where it is found | Wavenumber / cm⁻¹ | Appearance |
|---|---|---|---|
| C–H | alkyl groups, alkenes, arenes | 2850–3100 | sharp, medium |
| C=C | alkenes | 1620–1680 | medium |
| aromatic C=C | arenes | several peaks in the range 1450–1650 | variable |
| C=O | aldehydes, ketones, carboxylic acids, esters, amides, acyl chlorides and acid anhydrides | 1630–1820 | strong, sharp |
| O–H | alcohols, phenols | 3200–3600 | broad |
| O–H | carboxylic acids | 2500–3300 | very broad, overlaps C–H |
| N–H | amines, amides | 3300–3500 | medium, often two peaks |
| C≡N | nitriles | 2220–2260 | sharp, medium |
| C–O | alcohols, esters, carboxylic acids | 1000–1300 | strong, in the fingerprint region |
| C–F | fluoroalkanes | 1000–1350 | strong, in the fingerprint region |
| C–C | alkanes, alkyl chains | 750–1100 | weak, in the fingerprint region |
| C–X | haloalkanes (X = Cl, Br, I) | 500–800 | in the fingerprint region |
The O–H absorptions are broad because hydrogen bonding between molecules spreads the vibration over a range of frequencies; a carboxylic acid O–H is the broadest of all and runs into the C–H region.
An alcohol shows a broad O–H near 3350 and no C=O; a carboxylic acid shows both a very broad O–H and a strong C=O near 1715; an aldehyde or ketone shows the C=O but no O–H.
An alkene’s C=C is weaker than a C=O and is easy to miss.
The infrared spectra of ethanol and ethanoic acid with the O–H, C=O, C–H and C–O absorptions labelled and the fingerprint region shaded, beside the bonds to look up in the data you are given.
Exam focus: Write “absorption at 1630–1820 cm⁻¹ due to C=O”. The bond, the range from the OCR data sheet and the word absorption (or trough) are the three parts of the mark.
Check: Which Bond, Which Trough
Assign absorptions in spectra of compounds not discussed on this page.
The Fingerprint Region
Below about 1500 cm⁻¹ the spectrum contains many overlapping absorptions from bending vibrations and from C–C and C–O stretches.
This fingerprint region is too complicated to assign bond by bond, but its exact pattern is unique to each compound.
A computer compares the fingerprint region of an unknown with a database of spectra of pure compounds; an exact match identifies the compound and confirms its purity.
Key idea: Above 1500 cm⁻¹: identify the functional groups. Below 1500 cm⁻¹: match the fingerprint to a database.
Use the absorptions above 1500 cm⁻¹ to decide the functional group, then match the fingerprint region below 1500 cm⁻¹ against a database to identify the compound.
Check: Telling Compounds Apart
Use spectra to distinguish between compounds that are not the examples above.
Infrared in the Atmosphere and in Analysis
The same absorptions that make infrared spectroscopy useful cause the greenhouse effect. The Sun warms the Earth’s surface, which radiates the energy back as infrared.
The C=O bonds in carbon dioxide, the O–H bonds in water vapour and the C–H bonds in methane absorb some of that infrared, vibrate more energetically and pass the energy to other molecules by collision.
The atmosphere is warmed instead of the energy escaping to space. Water vapour is the largest natural contributor.
The rise in carbon dioxide from burning fossil fuels is thought to be the main cause of global warming, which has driven changes in energy use towards renewable sources and greater efficiency.
Infrared spectrometers are also used outside the laboratory. Modern breathalysers measure the ethanol in a breath sample from the size of its infrared absorption, and infrared analysers monitor air pollution, measuring carbon monoxide and nitrogen monoxide from vehicle exhausts by their characteristic absorptions.
Exam wording: “Infrared radiation emitted by the Earth is absorbed by the C=O bonds in CO₂ (and O–H in H₂O, C–H in CH₄), making the bonds vibrate; the energy is re-radiated or passed on by collisions and warms the atmosphere.”
Common Exam Points
Say
“A broad absorption at 3200–3600 cm⁻¹ shows an O–H group in an alcohol.” “No absorption at 1630–1820 cm⁻¹, so no C=O bond.” “The fingerprint region matches the database spectrum of the pure compound.”
Do not say
“A peak at 1700” (say absorption or trough, and quote the range). “The O–H peak” without saying alcohol or acid.
Watch for
Distinguishing questions: name the absorption that one compound has and the other lacks, with the wavenumber range.
Check: Predicting a Spectrum
Predict the absorptions of compounds not shown on this page.
FAQs
Use these quick answers to check infrared spectroscopy.
Why does the spectrum have troughs rather than peaks?
The y-axis is transmittance, the fraction of radiation that gets through. Where a bond absorbs, less radiation is transmitted, so the line dips.
Why is the O–H absorption broad?
Hydrogen bonding between molecules varies the strength of each O–H bond slightly, so the vibrations are spread over a range of wavenumbers. Carboxylic acids hydrogen bond most strongly and give the broadest band.
Can I tell an aldehyde from a ketone by infrared?
Not reliably. Both show the C=O absorption near 1700 cm⁻¹. Use the mass spectrum or a chemical test such as Tollens’ reagent or Fehling’s solution.
What is the fingerprint region for?
Matching. Below 1500 cm⁻¹ the pattern is unique to each compound, so comparing it with a database spectrum identifies the compound and shows whether it is pure.
Do I have to remember the wavenumbers?
No. The exam gives you the OCR data sheet; the skill is to look up the right bond and quote the range in your answer.
Copyright notice: This OLS revision content, including the explanations, layout, diagrams, tables and embedded learning structure, is authored for Online Learning System by Dr. Mohammed Al-Fatah. It may not be copied, reproduced, redistributed or adapted without written permission.
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