Atomic Absorption Spectroscopy

        Spec samplesAlanWalsh
        The begining of Atomic Absorption spectroscopy began with the chemist William Hyde Wollaston when he first absorbed absorption spectra of solar rays.  Later, Gustav Kirchhoff determined that the spectra lines were from the absorption of vapor's in the sun's atomosphere.  Talbot an Herschel laid the ground work for identifying compounds when they observed that a flames color would change when different compound salts were exposed to the flame.  Alan Walsh (pictured left) is credited for the establishment of the Atomic Absorption principle between 1952  and 1977 while working for the CSIR Division of Industrial Chemistry in Melbourne, Australia.   As we all have surely done on a Sunday afternoon, Alan began to wonder why Molecular spectra was found in absorption and Atomic Spectra in emission.  He began to think that the Absorption spectra had much more to offer.  He also thought that since the thermal source was more easily controlled there would be less inter-element interference then was currently being experienced in emission spectroscopy.  In his first experiments he used a sodium vapor lamp and a direct vision spectrometer.  The intensity was measured by a photomultiplier tube and recorded by a cathode ray oscillograph.  He sprayed sodium chloride solution over the simple flame and established the basis for atomic absorption spectroscopy.  He had difficuly reproducing the same resultd for other elements however and realized he needed a much stronger light source.  He came to the result of using hollow cathode lamps.  Alan Wlash had done it!  He developed the first atomic absorption spectrometer that had all the components now included in every AASpectrometer today!  They were a sealed hollow cathode lamp as the source, flame atomizer as the absorber, and a tuned amplifier.  For the full biographpy and development of AAS by walsh and his collegues please visit http://www.science.org.au/academy/memoirs/walsh2.htm#11.

        Atomic Absorption spectroscopy is specifically used to determine the concentration of a metal in a substance.  The concentrations are usually low and measured in mg/L.  AAS measures the absorption of light of the atoms of a substance in the gas phase. Flame AAS Therefore substance must first be dissolved in a liquid, dried and then atomized to vaporize the substance into gas atoms.  GraphiteFrunacePlease refer to the Sample Preparation page for more details on how toys are prepared for analysis.  There are two types of AAS equipment, Flame AAS and Graphite Furnace AAS. (pictured to the left anf right respectivly)  Flame AAS as the name states uses a flame to directly heat the sample and break it down into its gas phase.  Graphite Furnace AAS is generally electrically powered to heat a graphite column where the sample has been injected.  The graphite furnace AAS is generally more efficent, it can accept both liquid and organic samples and also in very small amounts.  The liquid samples are dried to ash and then atomized and the organic samples are reduced to ash and then atomized. 
      
        Once the sample has been atomized it is exposed to ultraviolet or visible light to determine the transitions of energy levels.  The light is absorbed by the electrons and moves them from their ground state to their excited state.  Transitional energies which are specific to compounds and elements lead to their identification are then directed to the detector where readings are recorded.  AASdiagram
Callibration of the spectrometer is of the utmost importance before these readings are taken.  Solutions of known concentrations should be run to establish a calibration curve which is compared to the unknowns and consequently identified.  The amount of light the sample finally absorbs will determine its concentration; calculations are made using the concepts of the Beer-Lambert Law.
      
        The Beer-Lambert Law is a logarithmic relation between the transmission (T) of light through the sample, the absorption coefficent (α
) of the sample and the path length ().
 T = {I\over I_{0}} = e^{-\alpha'\, l} = e^{-\sigma \ell N}

where I0 and I are the intensity of the incident light and the sample after energy has been absorbed.

References

http://www.spectroscopynow.com/coi/cda/detail.cda?page=2&id=1905&type=EducationFeature&chId=1

http://www.galbraith.com/spectroscopy.html

http://www.scribd.com/doc/10514011/Atomic-Absorption-Spectroscopy

http://www.bookrags.com/research/absorption-spectroscopy-woc/

http://www.science.org.au/academy/memoirs/walsh2.htm#8

http://www.files.chem.vt.edu/chem-ed/spec/atomic/aa.html



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