VISIBLE SPECTROPHOTOMETRY AND
COLORIMETRY
BY
DR. NEETU SONI ,SHUATS, PRAYAGRAJ
Instrumental visible spectroscopy is a
logical extension of the color tests and
visual observations. It is a sensitive,
accurate method of measuring the
colors or mixtures of colors that our
eyes perceive.
Spectrophotometry is the quantitative measurement
of how much a chemical substance absorbs light by
passing a beam of light through the sample using a
spectrophotometer. By measuring the intensity of
light detected, this method can be used to determine
the concentration of solute in the sample.
The visible light spectrum is the segment of
the electromagnetic spectrum that the
human eye can view. More simply, this range
of wavelengths is called visible light.
Typically, the human eye can detect
wavelengths from 380 to 700 nanometers.
Spectrophotometer
The spectrophotometer refers to an
instrument that measures the absorbance of
the test sample at a specific wavelength by
measuring the amount of light transmitted by
the sample. This device contains several
components like a light source, collimator,
monochromator, cuvette, light detector, and
digital meter.
Colorimetry is a scientific technique that
is used to determine the concentration of
colored compounds in solutions by the
application of the Beer–Lambert law,
which states that the concentration of a
solute is proportional to the absorbance.
Theory of spectrophotometry and
colorimetry
When light (monochromatic or heterogeneous) is
incident upon a homogeneous medium, a part of the
incident light is reflected, a part is absorbed by the
medium, and the remainder is transmitted as such.
Color comparison was one of the oldest methods
used for quantitative estimation of elements and
substances. The variation of a color of a system
with change in concentration of some components
forms the basis of colorimetric analysis.
In visual colorimetry, natural or artificial white light
(the whole range of the visible radiation is from
400-760 nm) is generally used as a light source
and determinations are usually made with a simple
instrument termed as colorimeter or color
comparator.
Lambert’s and Beer’s law.
When light (monochromatic or heterogeneous) is
incident upon a homogeneous medium, a part of the
incident light is reflected, a part is absorbed by the
medium, and the remainder is transmitted as such. If I0
denotes the intensity of the incident light, It, the
transmitted light, Ir the reflected light and Ia the
absorbed light, then it may be written:
I0 = Ia + It + Ir
Ir is very small then
I0 = Ia + It
Lambert’s law: When a monochromatic light passes through a
transparent medium, the rate of decrease in intensity (I) with thickness
(l) of the medium is proportional to the intensity of light.
Mathematically, –dI/dl∞I
On deduction it stands to It = I0 × e –kl (k is a proportionality constant)
On changing the above equation from natural to common logarithm,
It = I0 × 10–0.4343kl or
It = I0 × 10–Kl (K is called absorption coefficient)
The absorption coefficient is generally defined as the reciprocal of
the thickness (l cm.) required to reduce 1/10th of its intensity.
It/I0 = 0.1 = 10–Kl
or
K × l = 1
or
K = 1/l So unit of K is cm–1
The ratio (It/I0) is termed as Transmittance (T)
The ratio (I0/It) is termed as Opacity
log(I0/It)is termed as the Absorbance (A) of the medium or
Optical density (OD).
Beer’s law: When a beam of monochromatic light is allowed to pass
through a solution, the intensity of the light beam decreases
exponentially with the increase in concentration as well as thickness
of the solution. The equation becomes:
It = I0 × 10–a.c.l (a is called molar absorption coefficient)
The value of ‘a’ depends on the unit of concentration. If c is expressed in
gm-moles/litre, l in cm, then a is replaced by ε and is termed as molar
extinction coefficient.
The equation becomes: It = I0 × 10–ε.c.l
A = ε.c.l
or, ε = A/c.l
The unit of ε thus becomes litre gm-moles–1cm–1 Absorbance per unit
path length (l) per unit concentration (c) is known as specific extinction
coefficient
Instrumentation
All spectrophotomete, Photometers and Colorimeters have the following
basic components.
 Source of continuous radiation over the wavelengths of
interest.
 A Filter or Monochromator for selecting a narrow band of
wavelengths from the source spectrum.
Sample cell A container for the sample.
A Detector for converting radiant energy into electrical
energy, and
 A Read out system device to read out the response of the
detector.
The radiation source
Tungsten filament (300–2500 nm)
.
Filter
It can transmit or reflect a specified range of wavelength.
Filters are classified into three
types
Long wave pass filters,
Short wave pass filters
 Band pass filters
Types of filter from the viewpoint of function
(1) Absorption filter : a filter which absorbs a specific
range of wavelengths, for examples, colored filter
glass and gelatin filter.
(2) Interference filter : a filter which transmits a specific
range of wavelengths by utilizing the interference effect of
a thin film.
Prisms
A prism disperses polychromatic light from the source
into its constituent wavelengths by virtue of its ability to
reflect different wavelengths to a different extent
Two types of Prisms are usually employed in commercial
instruments. Namely, 600 cornu quartz prism and
300 Littrow Prism.
Grating
Gratings are often used in the monochromators of
spectrophotometers operating ultraviolet, visible and infrared
regions.
Monochromator
(1) entrance slit, (2) collimating mirror (to form a parallel beam after the slit),
(3) diffraction grating (dispersive element), (4) camera mirror (focuses light from
the dispersive element onto the exit slit), and (5) exit slit.
Detectors
Detectors are instruments that measure the amount of
ultraviolet or visible light absorbed by the sample
molecules.
In order to detect radiation three types of photosensitive
devices are
Photovoltaic cell
Phototubes
Photomultiplier
Photovoltaic cell
The Photovoltaic cell is the semiconductor device that converts the light
into electrical energy. The voltage induces by the PV cell depends on the
intensity of light incident on it.
Phototubes
Phototube is also known as a photoelectric cell.
It is filled with gas under low pressure.
It contains a light-sensitive cathode and anode inside an evacuated
quartz envelope.
A photon entering the tube strikes the cathode and leads to the ejection
of an electron.
 Electrons strikes the anode and results in the flow of current. The
resulting current is of low intensity and requires amplification.
The response in the phototube depends on the wavelength of incident
light.
Phototubes
Photomultiplier tube is used in UV-Vis spectrophotometers.
 It has an anode, cathode, and many dynodes.
Photon when entering the tube, strikes the cathode, resulting in
the emission of electrons.
The emitted electrons are accelerated towards the first dynode,
An electron striking the first dynode will result in the production of
several electrons.
The process repeats itself continuously from one dynode to
another and after passing to 10 dynodes.
Photomultiplier Tube
A colorimeter is an instrument that compares the amount of
light getting through a solution with the amount that can get
through a sample of pure solvent.
Visual comparators
•Multiple standard method
•Duplication Method
•Dilution methods
•Balancing method
Colorimeter
Dubosq colorimeter
Application of colorimetry and
spectrophotometry:
(i) Determination of molar composition of complexes.
(ii) Determination of instability constants of complexes.
(iii) Determination of pK value of an indicator.
(iv) Elucidation of structures of organic as well as
inorganic compounds.
(v) Determination of molecular weight of colored
substances.

Visible Spectrophotometry and Colorimetry.pptx

  • 1.
  • 2.
    Instrumental visible spectroscopyis a logical extension of the color tests and visual observations. It is a sensitive, accurate method of measuring the colors or mixtures of colors that our eyes perceive.
  • 3.
    Spectrophotometry is thequantitative measurement of how much a chemical substance absorbs light by passing a beam of light through the sample using a spectrophotometer. By measuring the intensity of light detected, this method can be used to determine the concentration of solute in the sample.
  • 5.
    The visible lightspectrum is the segment of the electromagnetic spectrum that the human eye can view. More simply, this range of wavelengths is called visible light. Typically, the human eye can detect wavelengths from 380 to 700 nanometers.
  • 6.
    Spectrophotometer The spectrophotometer refersto an instrument that measures the absorbance of the test sample at a specific wavelength by measuring the amount of light transmitted by the sample. This device contains several components like a light source, collimator, monochromator, cuvette, light detector, and digital meter.
  • 7.
    Colorimetry is ascientific technique that is used to determine the concentration of colored compounds in solutions by the application of the Beer–Lambert law, which states that the concentration of a solute is proportional to the absorbance.
  • 9.
    Theory of spectrophotometryand colorimetry When light (monochromatic or heterogeneous) is incident upon a homogeneous medium, a part of the incident light is reflected, a part is absorbed by the medium, and the remainder is transmitted as such. Color comparison was one of the oldest methods used for quantitative estimation of elements and substances. The variation of a color of a system with change in concentration of some components forms the basis of colorimetric analysis.
  • 10.
    In visual colorimetry,natural or artificial white light (the whole range of the visible radiation is from 400-760 nm) is generally used as a light source and determinations are usually made with a simple instrument termed as colorimeter or color comparator.
  • 11.
    Lambert’s and Beer’slaw. When light (monochromatic or heterogeneous) is incident upon a homogeneous medium, a part of the incident light is reflected, a part is absorbed by the medium, and the remainder is transmitted as such. If I0 denotes the intensity of the incident light, It, the transmitted light, Ir the reflected light and Ia the absorbed light, then it may be written: I0 = Ia + It + Ir Ir is very small then I0 = Ia + It
  • 12.
    Lambert’s law: Whena monochromatic light passes through a transparent medium, the rate of decrease in intensity (I) with thickness (l) of the medium is proportional to the intensity of light. Mathematically, –dI/dl∞I On deduction it stands to It = I0 × e –kl (k is a proportionality constant) On changing the above equation from natural to common logarithm, It = I0 × 10–0.4343kl or It = I0 × 10–Kl (K is called absorption coefficient) The absorption coefficient is generally defined as the reciprocal of the thickness (l cm.) required to reduce 1/10th of its intensity. It/I0 = 0.1 = 10–Kl or K × l = 1 or K = 1/l So unit of K is cm–1
  • 13.
    The ratio (It/I0)is termed as Transmittance (T) The ratio (I0/It) is termed as Opacity log(I0/It)is termed as the Absorbance (A) of the medium or Optical density (OD).
  • 14.
    Beer’s law: Whena beam of monochromatic light is allowed to pass through a solution, the intensity of the light beam decreases exponentially with the increase in concentration as well as thickness of the solution. The equation becomes: It = I0 × 10–a.c.l (a is called molar absorption coefficient) The value of ‘a’ depends on the unit of concentration. If c is expressed in gm-moles/litre, l in cm, then a is replaced by ε and is termed as molar extinction coefficient. The equation becomes: It = I0 × 10–ε.c.l A = ε.c.l or, ε = A/c.l The unit of ε thus becomes litre gm-moles–1cm–1 Absorbance per unit path length (l) per unit concentration (c) is known as specific extinction coefficient
  • 15.
    Instrumentation All spectrophotomete, Photometersand Colorimeters have the following basic components.  Source of continuous radiation over the wavelengths of interest.  A Filter or Monochromator for selecting a narrow band of wavelengths from the source spectrum. Sample cell A container for the sample. A Detector for converting radiant energy into electrical energy, and  A Read out system device to read out the response of the detector.
  • 16.
    The radiation source Tungstenfilament (300–2500 nm) . Filter It can transmit or reflect a specified range of wavelength. Filters are classified into three types Long wave pass filters, Short wave pass filters  Band pass filters
  • 17.
    Types of filterfrom the viewpoint of function (1) Absorption filter : a filter which absorbs a specific range of wavelengths, for examples, colored filter glass and gelatin filter. (2) Interference filter : a filter which transmits a specific range of wavelengths by utilizing the interference effect of a thin film.
  • 18.
    Prisms A prism dispersespolychromatic light from the source into its constituent wavelengths by virtue of its ability to reflect different wavelengths to a different extent Two types of Prisms are usually employed in commercial instruments. Namely, 600 cornu quartz prism and 300 Littrow Prism.
  • 19.
    Grating Gratings are oftenused in the monochromators of spectrophotometers operating ultraviolet, visible and infrared regions.
  • 20.
    Monochromator (1) entrance slit,(2) collimating mirror (to form a parallel beam after the slit), (3) diffraction grating (dispersive element), (4) camera mirror (focuses light from the dispersive element onto the exit slit), and (5) exit slit.
  • 21.
    Detectors Detectors are instrumentsthat measure the amount of ultraviolet or visible light absorbed by the sample molecules. In order to detect radiation three types of photosensitive devices are Photovoltaic cell Phototubes Photomultiplier
  • 22.
    Photovoltaic cell The Photovoltaiccell is the semiconductor device that converts the light into electrical energy. The voltage induces by the PV cell depends on the intensity of light incident on it.
  • 23.
    Phototubes Phototube is alsoknown as a photoelectric cell. It is filled with gas under low pressure. It contains a light-sensitive cathode and anode inside an evacuated quartz envelope. A photon entering the tube strikes the cathode and leads to the ejection of an electron.  Electrons strikes the anode and results in the flow of current. The resulting current is of low intensity and requires amplification. The response in the phototube depends on the wavelength of incident light.
  • 24.
  • 25.
    Photomultiplier tube isused in UV-Vis spectrophotometers.  It has an anode, cathode, and many dynodes. Photon when entering the tube, strikes the cathode, resulting in the emission of electrons. The emitted electrons are accelerated towards the first dynode, An electron striking the first dynode will result in the production of several electrons. The process repeats itself continuously from one dynode to another and after passing to 10 dynodes. Photomultiplier Tube
  • 28.
    A colorimeter isan instrument that compares the amount of light getting through a solution with the amount that can get through a sample of pure solvent. Visual comparators •Multiple standard method •Duplication Method •Dilution methods •Balancing method Colorimeter
  • 29.
  • 31.
    Application of colorimetryand spectrophotometry: (i) Determination of molar composition of complexes. (ii) Determination of instability constants of complexes. (iii) Determination of pK value of an indicator. (iv) Elucidation of structures of organic as well as inorganic compounds. (v) Determination of molecular weight of colored substances.