Spectroscopy

Introduction

Spectroscopy is based on the interaction of electromagnetic radiation with matter.  Different wavelengths, λ (or frequencies ν), of light interact with different physical properties of matter.

Electromagnetic Radiation (EMR)

The electromagnetic Spectrum

There is a continuum of wavelength (or frequency) of EMR.  Different wavelengths will interact with different physical properties of matter.  This results in a number of different Spectroscopy methods.

EMR has both wave-like properties and particle-like properties.
Wave-like properties:
Depends on the wavelength (λ), frequency (ν) and are related by the speed of light(c): c = λ ν or λ = c / ν or ν = c / λ
(c is the speed of light: 3 x 108 m/s)
Particle-like properties:
Depend on the quantized energy of a photon where the energy is given by: E = h ν = h c / λ
(h = Plank's constant 6.626 x 10-34 Js)
Note that the energy is directly proportional to the frequency and inversely proportional to the wavelength.

Excited States

All spectroscopy methods rely on the molecule absorbing energy and moving from a ground energy state to an excited energy state.  We can measure the amount and frequency of energy absorbed which will correspond to specific physical features in the molecules.  For example, the absorption of energy by an electron in the ground state will result in an excited electronic state (see image right).

electronic excitation in UV-Vis spectroscopy
The longest wavelength (lowest frequency) have the least amount of energy. 
IR Spectroscopy NMR Spectroscopy Mass Spectrometry (MS) UV-Vis Spectroscopy
1H-NMR 13C-NMR
Geting Structures from Spectra

Test your knowledge

IR , 1H-NMR, 13C-NMR, MS and UV-Vis
Examples of Structure Determination
More Structure Determination Problems

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