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IR SpectroscopyLoad the IR Spectrum Alcohols are easily recognized by the broad, strong O-H stretching band between 3300-3500 cm-1. Note that this is a different band from the (usually present) C-H bands around 3000 cm-1. Most other bands are complex vibrations of the molecule. Click on any IR peak to see what vibration is activated by absorption at that frequency. The O-H peak here is abnormally sharp for an alcohol (the spectrum is actually collected in the gas phase). See several examples below for more "normal" solution behavior. |
1H NMR SpectroscopyLoad the 1H NMR There are two signals of interest. The O-H proton is highly variable in its chemical shift, but is normally broad (due to H-bonding) and not coupled to other protons except under special circumstances. A significant experiment is D2O exchange; the deuterium will exchange with the OH; the signal will move or disappear altogether. The second signal is that for any proton on the oxygen-bearing carbon; this will occur between 3.5-4.5 ppm and will couple normally to its neighbors (but not usually to the OH). Again, click on any signal to highlight the proton responsible for it. |
13C NMR SpectroscopyLoad the 13C NMR spectrum Carbons bearing an oxygen are deshielded and normally occur in the 60-80 ppm region; a carbon with more than one oxygen may be further downfield. Other carbons in this molecule occur further upfield, as they should. The oxygen exerts a slight influence on those closest. Select each signal to see which carbon generates it. Mass spectrometryLoad mass spectrumThe radical cations of alcohols easily lose water; here, the first major fragment lost is a methyl group via a process called "α-cleavage" to give a peak at m/z = 73. Cleavage on the other side of the alcohol leads to loss of a propyl group at m/z = 45 to give the largest peak in the spectrum. |