Chemistry Net: Analytical Chemistry - Atomic Absorption
Showing posts with label Analytical Chemistry - Atomic Absorption. Show all posts
Showing posts with label Analytical Chemistry - Atomic Absorption. Show all posts

Analytical Chemistry - Atomic Absorption

Atomic Absorption

ATOMIC ABSORPTION

 

 

 

 

 

 

 

 

Atomic absorption spectrometry (AAS) is an analytical technique that measures the concentration of an element by measuring the amount of light (intensity of light) that is absorbed - at a characteristic wavelength - when it passes through a cloud of atoms of this element. As the number of atoms in the light path increases, the amount of light absorbed increases in a predictable way. Modern atomic absorption spectrometry was introduced in 1955 as a result of the independent work  of A. Walsh and C.T.J Alkemade. Commercial atomic absorption spectrophotometers were introduced by the early 1960’s, and the importance of atomic absorption as an analytical technique was soon evident.

 


References

  1. (a) A. Walsh, Anal. Chem., 63, 933A–941A, 1991 (b) S.R. Koirtyohann, Anal. Chem., 63, 1024A–1031A, 1991 (c) W. Slavin, Anal. Chem., 63, 1033A–1038A, 1991.

  2. D. Harvey,  “Modern Analytical Chemistry”, McGraw-Hill Companies Inc., 2000

  3. D.A. Skoog, F.J.  Holler, T.A.  Nieman,  “Principles of Instrumental Analysis”. Saunders College Publishing: Philadelphia, 1998.


Advantages and Disadvantages of Atomic Absorption Spectrometry and Graphite Furnace

Advantages and Disadvantages of Atomic Absorption Spectrometry and Graphite Furnace

 

Advantages and Disadvantages of Atomic Absorption Spectrometry and Graphite Furnace

Atomic Absorption Spectrometry (AAS) is an analytical technique that measures the concentration of an element by measuring the amount of light (intensity of light) that is absorbed - at a characteristic wavelength - when it passes through a cloud of atoms of this element.

As the number of atoms in the light path increases, the amount of light absorbed increases in a predictable way.

The main advantages of AAS  are given below:

  • High sample throughput
  • Easy to use
  • High precision
  • Inexpensive technique

The main disadvantages of AAS  are as follows:

  • only solutions can be analyzed
  • less sensitivity compared to graphite furnace
  • relatively large sample quantities are required (1-3 ml)
  • problems with refractory elements

 

Graphite furnace is by far the most advanced and widely used high sensitivity sampling technique for atomic absorption .

The main advantages of graphite furnace (GFAAS) over AAS can be summarized as follows:

  • Slurries and solid samples can be analyzed in addition to samples in solution
  • It shows greater sensitivity than AAS
  • Smaller quantities of sample are required (normally 5-60 μL)
  • The atomization process is more efficient comparing to AAS

The main disadvantages of  graphite furnace are given :

  • It is an expensive technique
  • Low sample throughput
  • It requires experienced operators.

 


Relevant Posts

Atomic Absorption Spectrometry (AAS)

Sampling Techniques for Atomic Absorption Spectrometry

 


References

  1. (a) A. Walsh, Anal. Chem., 63, 933A–941A, 1991 (b) S.R. Koirtyohann, Anal. Chem., 63, 1024A–1031A, 1991 (c) W. Slavin, Anal. Chem., 63, 1033A–1038A, 1991.
  2. D. Harvey,  “Modern Analytical Chemistry”, McGraw-Hill Companies Inc., 2000
  3. D.A. Skoog, F.J.  Holler, T.A.  Nieman,  “Principles of Instrumental Analysis”. Saunders College Publishing: Philadelphia, 1998.

Sampling Techniques for Atomic Absorption Spectrometry

Sampling Techniques for Atomic Absorption Spectrometry

Sampling Techniques for Atomic Absorption Spectrometry

 

Fig. I.1: A burner system used in atomic absorption spectrometers

Two systems are commonly used to produce atoms from the sample in atomic absorption spectrometry:

  • Aspiration
  • &

  • electrothermal atomization (graphite furnace).

 Aspiration involves sucking a solution of the sample into a flame. Figure I.1 shows a typical burner and spray chamber. Ethylene/air or ethylene /dinitrogen oxide are used. A flexible capillary tube connects the solution to the nebulizer. At the tip of the capillary, the solution is “nebulized” that means is broken into small drops. The larger drops fall out and drain off while smaller ones vaporize in the flame. Only 1% of the sample is nebulized.

 

Electrothermal atomization (graphite furnace, GFAAS) is where a drop of sample is placed into a graphite tube that is then heated electrically. This is by far the most advanced and widely used high sensitivity sampling technique for atomic absorption known also as graphite furnace. In this technique, a tube of graphite is located in the sample compartment of the atomic absorption spectrometer, with the light path passing through it. A small volume of the sample solution quantitatively placed into the tube through a sample injection hole located in the center of the tube wall. The tube is heated through a programmed temperature sequence until finally the analyte present in the sample is dissociated into atoms and atomic absorption occurs.

There are several advantages of the graphite furnace technique comparing to aspiration:

Fig. I.2: Graphite tube. A drop of sample is placed into the graphite tube and then is heated electrically. Since almost all the sample is dissociated into atoms a high concentration of atoms is obtained. This is by far the most advanced and widely used high sensitivity sampling technique for atomic absorption known also as graphite furnace.

  • The detection limits for the graphite furnace  fall in the ppb range (ng/l) for most elements. The sample is atomized in a very short period of time, concentrating the available atoms in the heated cell and resulting in the observed increased sensitivity.
  • The graphite furnace is much more automated than the other techniques. Even though heating programs can be very sophisticated, the entire process is automated once the sample has been introduced and the furnace program initiated. Automatic samplers are used to facilitate the process that can be completed unattended.
  • Interference problems have been minimized with the development of improved instrumentation
  • The graphite furnace can determine most elements measurable by AA in a wide variety of matrices.

 


Relevant Posts

Atomic Absorption Spectrometry (AAS)

Light sources for atomic absorption

 


References

  1. (a) A. Walsh, Anal. Chem., 63, 933A–941A, 1991 (b) S.R. Koirtyohann, Anal. Chem., 63, 1024A–1031A, 1991 (c) W. Slavin, Anal. Chem., 63, 1033A–1038A, 1991.
  2. D. Harvey,  “Modern Analytical Chemistry”, McGraw-Hill Companies Inc., 2000
  3. D.A. Skoog, F.J.  Holler, T.A.  Nieman,  “Principles of Instrumental Analysis”. Saunders College Publishing: Philadelphia, 1998.

 


Light sources for atomic absorption

Light sources for atomic absorption

Light sources for atomic absorption

It is well known that an atom in its ground state absorbs light at discrete wavelengths (E = h*c/λ). In order to measure this narrow light absorption with maximum sensitivity, it is necessary to use a line source, which emits the specific wavelengths which can be absorbed by the atom. Narrow line sources not only provide high sensitivity, but also make atomic absorption a very specific analytical technique.

The two most common line sources used in atomic absorption are the “hollow cathode lamp, HCL” and the “electrodeless discharge lamp, EDL”.

 

The Hollow Cathode Lamp HCL

The common source of light is a “hollow cathode lamp”. This contains a tungsten anode and a cylindrical hollow cathode made of the element to be determined. These are sealed in a glass tube filled with an inert gas – e.g. argon or neon – at a pressure between 1Nm-2 – 5Nm-2. 

When an electrical potential is applied between the anode and cathode, some of the inert gas atoms are ionized. These gaseous ions bombard the cathode and eject metal atoms from the cathode in a process called sputtering (Fig. I.1). Some sputtered atoms are in excited states and emit radiation characteristic of the metal as they fall back to the ground state. The shape of the cathode concentrates the radiation into a beam which passes through a quartz window, and the shape of the lamp is such that most of the sputtered atoms are redeposited on the cathode.

Hollow cathode lamps have a finite lifetime. With extended use, the sputtering process removes some of the metal atoms from the cathode and these are deposited elsewhere.

 

Fig. I.1: Hollow cathode lamp emission process

 

The Electrodeless Discharge Lamp  (EDL)

For most elements, the hollow cathode lamp is a completely satisfactory source for atomic absorption. In a few cases, however  such as the more volatile elements, the quality of the analysis is impaired by limitations of the hollow cathode lamp.

In cases like the above the electrodeless discharge lamp (EDL) is used. A small amount of the metal or salt of the element for which the source is to be used is sealed inside a quartz bulb. The bulb is placed inside a small, self-contained RF generator. When power is applied to the RF generator, an RF field is created. The energy will vaporize and excite the atoms, inside the bulb, causing them to emit their characteristic spectrum. Electrodeless discharge lamps are typically much more intense and in some cases, more sensitive than comparable hollow cathode lamps. They therefore offer a better precision and lower detection limits.


Relevant Posts

Atomic Absorption Spectrometry (AAS)

Quantitative Analysis by Atomic Absorption

 


References

  1. (a) A. Walsh, Anal. Chem., 63, 933A–941A, 1991 (b) S.R. Koirtyohann, Anal. Chem., 63, 1024A–1031A, 1991 (c) W. Slavin, Anal. Chem., 63, 1033A–1038A, 1991.
  2. D. Harvey,  “Modern Analytical Chemistry”, McGraw-Hill Companies Inc., 2000
  3. D.A. Skoog, F.J.  Holler, T.A.  Nieman,  “Principles of Instrumental Analysis”. Saunders College Publishing: Philadelphia, 1998.

Quantitative Analysis by Atomic Absorption

Quantitative Analysis by Atomic Absorption

 

Quantitative Analysis by Atomic Absorption

 

The capability of an atom to absorb very specific wavelengths of light is utilized in atomic absorption spectrometry.

Light of a specific wavelength and of initial intensity Io is focused on the flame cell containing ground state atoms. The initial light intensity is decreased by an amount determined by the atom concentration in the flame cell. The light is then directed to the detector where the reduced intensity, It, is measured. The amount of light absorbed is determined by comparing It  to Io and according to Beer’s law:

 

A = log Io / It = α * c * d         (1)

 

Absorbance A is the most convenient term for characterizing light absorption in absorption spectrophotometry, as this quantity follows a linear relationship with concentration c.

Equation (1) can be used for quantitative analysis by atomic absorption spectrometry AAS. A calibration curve is used to determine the unknown concentration of an element – i.e. nickel – in a solution. The instrument is calibrated using several solutions of known concentrations of the element under examination. The calibration curve shows the concentration of the element in solution against the amount of radiation absorbed (Fig. I.1).

The sample solution is fed into the instrument and the unknown concentration of the element  – i.e. nickel – is then displayed on the calibration curve (Fig. I.1).

For example for the Ni solution above an absorbance of 0.37 was obtained that corresponds to a concentration of 12 mg/l.

Over the region where the Beer’s law relationship is observed, the calibration yields a straight line. As the concentration and absorbance increase, nonideal behavior in the absorption process can cause a deviation from linearity as shown in Fig. I.1. There are several reasons for this nonideal behavior  such as nonhomogeneities of temperature and space in the absorbing cell, line broadening, absorption at nearby lines and stray light.

As shown above, after such a calibration is established (Fig. I.1) the absorbance of solutions of unknown concentrations may be measured and the corresponding concentrations can be determined from the calibration curve.

The instrument performance for an element can be monitored by the following parameters:

  • Characteristic concentration for the element
  • Detection limit

The characteristic concentration for an element (called “sensitivity”) is a convention and is defined as the concentration of analyte giving an absorbance of 0.00436 (corresponding to a percent transmittance of 99%). Usually the wavelength providing the best sensitivity is used, although a less sensitive wavelength may be more appropriate for a high concentration of analyte. A less sensitive wavelength also may be appropriate when significant interferences occur at the most sensitive wavelength.

 

Characteristic Conc. (mg/l) = Conc. of Standard (mg/l) * 0.0044  /  measured absorbance

 

There are several practical reasons for wanting to know the value of the characteristic concentration for an element. For example, knowing the expected characteristic concentration of an element allows an operator to determine if all instrumental conditions are optimized and if the instrument is performing according to specifications. This is accomplished by simply measuring the absorbance of a known concentration of the element and comparing the results to the expected value.

Even though the magnitude of the absorbance signal can be predicted from the value given for characteristic concentration, no information is given on how small of an absorbance signal can be measured.

The smallest measurable concentration of an element – the detection limit of the element -  will be determined by the magnitude of the absorbance observed for the element and the stability of the absorbance signal.

The detection limit (according to IUPAC) is the smallest concentration or absolute amount of analyte that has a signal significantly larger than the signal arising from a reagent blank.

Mathematically, the analyte’s signal at the detection limit (sDL) is given by:

 

sDL = sreag + 3 * σreag

where sreag is the signal for a reagent blank, sreag is the known standard deviation for the reagent blank’s signal.

Other approaches for defining the detection limit have also been developed. In atomic absorption spectrometry usually the detection limit is determined for a certain element by analyzing a diluted solution of this element and recording the corresponding absorbances. The experiment is repeated for 10 times. The 3σ of the recorded absorbance signal can be considered as the detection limit for the specific element under the experimental conditions used – wavelength, type of flame, instrument.

For example, let us suppose that the detection limit for Cu has to be determined by AAS under certain experimental conditions. A 0.1 ppm Cu solution is analyzed for 10 times by AAS at a wavelength of 324.8 nm and the corresponding absorbance values are recorded:


Experiment #
Absorbace
1
0.006
2
0.005
3
0.007
4
0.007
5
0.006
6
0.007
7
0.005
8
0.004
9
0.005
10
0.004
Average
0.0056
σ
0.0012
0.0036

 

Therefore, the detection limit for Cu (Cu signal at the detection limit) under the above conditions is 0.0036 and this absorbance corresponds to a Cu solution concentration approximately at:

0.1 ppm * (0.0036/0.0056) = 0.064 ppm (assuming we are working on the linear region of the calibration curve).


Relevant Posts

Atomic Absorption Spectrometry (AAS)

Advantages and Disadvantages of Atomic Absorption Spectrometry and Graphite Furnace

 


References

  1. R. Ferrus, ; M.R. Egea, Anal. Chim. Acta, 287, 119–145 (1994)
  2. J.A. Glaser, D.L. Foerst, et al. Environ. Sci.Technol., 15, 1426–1435 (1981)
  3. P.W.J. Boumans, Anal. Chem., 66, 459A–467A (1994)

Atomic Absorption Spectrometry (AAS)

Atomic Absorption Spectrometry (AAS)

Atomic Absorption Spectrometry (AAS)

 

Atomic absorption spectrometry (AAS) is an analytical technique that measures the concentration of an element by measuring the amount of light (intensity of light) that is absorbed - at a characteristic wavelength - when it passes through a cloud of atoms of this element.

As the number of atoms in the light path increases, the amount of light absorbed increases in a predictable way.

 

History of Atomic Absorption Spectrometry

The phenomenon of light absorption had already been investigated at the beginning of the 18th century. It was observed that the original radiation intensity is resolved into three components: into reflected, transmitted and absorbed radiation.

The two fundamental laws governing the fraction of incident radiation absorbed on passing through a sample are the Lambert’s law (1768) and the Beer’s law (1852).

The first law, was stated by Bouguer in 1729 and restated by Lambert in 1768 is called the Lambert’s law and predicts the effect of thickness of a sample medium upon the fraction of radiation which is absorbed. Lambert reached the intuitively reasonable conclusion that each unit length of material through which radiation passes absorbs the same fraction of radiation. If for example a monochromatic beam of intensity Io passes through a thickness d of absorbing material the transmitted beam intensity It will be reduced and will be equal with:

It  =  Io * e-k.d             (1)

The proportionality constant k is called absorption coefficient and depends on the wavelength and the temperature of a given substance.

Lambert’s law (1) is an exact law and applies to any homogeneous, nonscattering medium, regardless of whether it is a gas, liquid, solid or solution.

Lambert’s law underwent a thorough examination by Beer and he proposed a more useful law for chemistry:

A = log Io / It = α * c * d       (2)

It states that the absorbance A is proportional to the concentration c of the absorbing substance and to the thickness d of the absorbing layer. The constant α is a new proportionality constant.

 

The Atomic Absorption Process

If light of just the right wavelength strikes on a free, ground state atom, the atom absorbs the light as it enters in an excited state. This process is called atomic absorption and is illustrated in Fig. I.1:

 

Fig. I.1: The atomic absorption process. The atom absorbs light of a specific wavelength (specific amount of energy) and it goes to an excited state

 

The capability of an atom to absorb very specific wavelengths of light is utilized in atomic absorption spectrometry.

Light of a specific wavelength and of initial intensity Io is focused on the flame cell containing ground state atoms. The initial light intensity is decreased by an amount determined by the atom concentration in the flame cell. The light is then directed to the detector where the reduced intensity, It, is measured. The amount of light absorbed is determined by comparing It  to Io and according to Beer’s law:

A = log Io / It = α * c * d       (2)

Absorbance A is the most convenient term for characterizing light absorption in absorption spectrophotometry, as this quantity follows a linear relationship with concentration.

 

Atomic Absorption Spectrophotometer

Modern atomic absorption spectrometry was introduced in 1955 as a result of the independent work  of A. Walsh and C.T.J Alkemade. Commercial atomic absorption spectrophotometers were introduced by the early 1960’s, and the importance of atomic absorption as an analytical technique was soon evident. Perkin-Elmer has been the undisputed global leader in AAS for over 50 years.

There are five basic components of an atomic absorption instrument: The light source, an “absorption cell”, a monochromator, a detector and a screen.

The light source that emits light of a specific frequency for the element under investigation. The light source is usually a hollow cathode lamp or an electrodeless  discharge lamp. The light source is electronically modulated or mechanically chopped to differentiate between the light from the source and the emission from the sample cell.

An “absorption cell” in which atoms of the sample are produced (flame, graphite furnace, FIAS cell, FIMS cell, MHS cell). When flame atomization is used the sample is first converted into a fine mist consisting of small droplets of solution. This is accomplished by using a nebulizer assemply. Subsequently, thermal energy volatizes the particles producing a vapor consisting of molecular species, ionic species and free atoms. Thermal energy in flame atomization is provided by the combustion of a fuel-oxidant mixture. Air-acetylene (temperature: 2100-2400 C) and nitrous oxide – acetylene flames (temperature: 2600-2800  C) are used most frequently.

 

Fig. I.2: The basic components of an atomic absorption instrument

 

A monochromator for light dispersion. The monochromator is used to select the specific wavelength of light – a spectral line – which is absorbed by the sample, and to exclude other wavelengths. The selection of the specific light allows the determination of the selected element in the presence of others. The light selected by the monochromator is directed onto a detector that is a photomultiplier tube. This produces an electrical signal proportional to the light intensity.

A detector, which measures the light intensity and amplifies the signal.

A screen that shows the reading after it has been processed by the instrument.

 

Uses of Atomic Absorption Spectrometry

Atomic absorption spectrometry has many uses in different areas of chemistry such as:

  • Clinical analysis: Analyzing metals in biological fluids and tissues such as whole blood, plasma, urine, saliva, brain tissue, liver, muscle tissue, semen, umbilical cord.
  • Pharmaceuticals: In some pharmaceutical manufacturing processes, minute quantities of a catalyst that remain in the final drug product, active pharmaceutical ingredient.
  • Water analysis: Analyzing water for its metal content
  • Food Analysis: The technique is increasingly being used in the food and beverage industries to ensure compliance with stringent global legislation. Combining flame, furnace, and vapor techniques, atomic absorption spectrophotometry facilitates the analysis of a large number of toxic trace elements across a wide analytical range, from parts per million (ppm) down to subparts per billion (ppb).
  • Mining: By using AAS the amount of metals such as gold in rocks can be determined to see whether it is worth mining the rocks to extract precious metals 

 


Relevant Posts

Sampling techniques for atomic absorption spectrometry

Light sources for atomic absorption

Quantitative analysis by atomic absorption

Advantages and disadvantages atomic absorption and graphite furnace


References

  1. (a) A. Walsh, Anal. Chem., 63, 933A–941A, 1991 (b) S.R. Koirtyohann, Anal. Chem., 63, 1024A–1031A, 1991 (c) W. Slavin, Anal. Chem., 63, 1033A–1038A, 1991.
  2. D. Harvey,  “Modern Analytical Chemistry”, McGraw-Hill Companies Inc., 2000
  3. D.A. Skoog, F.J.  Holler, T.A.  Nieman,  “Principles of Instrumental Analysis”. Saunders College Publishing: Philadelphia, 1998.