SlideShare a Scribd company logo
1 of 25
UV VISIBLE
SPECTROSCOPY
S.PRAVALIKA
170417881067
SNVPMV
CONTENTS:
 Introduction
 Electronic transitions
 Chromophores
 Auxochromes
 Spectral shifts
 Solvent effect on absorption spectra
INTRODUCTION
 Spectroscopy is the branch of science that deals with the study of
interaction of electromagnetic radiation with matter.
 It is the most powerful tool available for the study of atomic & molecular
structure and is used in the analysis of a wide range of samples. The two
main types are:
 Atomic Spectroscopy; This Spectroscopy is concerned with the interaction
of electromagnetic radiation with atoms which are commonly in the lowest
energy state called as ground state.
 Molecular Spectroscopy ; This Spectroscopy deals with the interaction of
electromagnetic radiation with molecule.
 • Electromagnetic radiation consist of discrete packets of energy which are
called as photons.
 • A photon consists of an oscillating electric field (E) & an oscillating
magnetic field (M) which are perpendicular to each other.
Wavelength (, lambda): Distance from one wave peak to the next.
Units: m, cm, m, nm
Frequency (, nu): Number of peaks that pass through a given point per
second.
Units: Cycles/second or s-1 or Hertz (Hz)
Wave number
Number of waves per cm.
ELECTRONIC
TRANSITIONS
1)σ → σ* transition.
 σ electron from orbital is excited to corresponding anti-bonding
orbital σ*.
 The energy required is large for this transition.
 e.g. Methane (CH4) has C-H bond only and can undergo σ → σ*
transition and shows absorbance maxima at 125 nm.
2) π → π* transition
• π electron in a bonding orbital is excited to corresponding anti-
bonding orbital π*.
• Compounds containing multiple bonds like alkenes, alkynes,
carbonyl, nitriles, aromatic compounds, etc undergo π → π*
transitions.
• e.g. Alkenes generally absorb in the region 170 to 205 nm.
3) n → σ* transition
• Saturated compounds containing atoms with lone pair of
electrons like O, N, S and halogens are capable of n → σ*
transition.
• These transitions usually requires less energy than σ → σ*
transitions.
• The number of organic functional groups with n → σ* peaks
in UV region is small (150 – 250 nm).
4) n → π* transition
• An electron from non-bonding orbital is promoted to anti-
bonding π* orbital.
• Compounds containing double bond involving hetero atoms
(C=O, C≡N, N=O) undergo such transitions.
• n → π* transitions require minimum energy and show
absorption at longer wavelength around 300 nm.
5) & 6) σ → π* transition & π → σ* transition .
 These electronic transitions are forbidden transitions & are only
theoretically possible.
 Thus, n → π* & π → π* electronic transitions show absorption in
region above 200 nm which is accessible to UV-visible
spectrophotometer.
CHROMOPHORES
 Defined as any isolated covalently bonded group that shows a
characteristic absorption of Electromagnetic radiation in the UV or
visible region.
 It is a Greek word. Chroma = “color” & phoros = “bearer”
Compound containing chromophore is CHROMOGEN
 Eg: C=C, C=O, NO2
TYPES OF CHROMOPHORES
 1. INDEPENDENT CHROMOPHORES: If one chromophore is
required to impart colour Eg: Azo group –N=N-, Nitroso group –
NO-
 2. DEPENDENT CHROMOPHORES: If more than one
chromophore is required to impart colour Eg: Acetone having one
ketone group is colorless whereas diacetyl having two ketone
groups is yellow.
 Identification of a chromophore depends on a number of factors as
follows;
 i) Spectrum consisting of a band near 300 mµ may contain two or
three conjugated units.
 ii) Absorption bands near 270-350 mµ with very low intensity εmax
10-100 are due to n → π*transitions of the carbonyl group.
 iii) Simple conjugated chromophores such as dienes or α, β-
unsaturated ketones have high εmax values, i.e., 10,000 to 20,000.
AUXOCHROMES
 Auxochrome: A saturated/ unsaturated group with non
bonding electrons when attached to chromophore altering
both wavelength as well as intensity of absorption.
Eg: OH, NH2, NHR, COOH, CN, Cl etc..
Two types:
1) Basic/positive auxochromic groups Effective in acid
solutions
 Eg: OH, OR, NHR etc.
2) Acidic/negative auxochromic groups Effective in alkaline
solutions
 Eg: NO, CO, CN etc.
SPECTRAL SHIFTS
 Substituents may have any of four effects on a
chromophore :
i. Bathochromic shift (red shift) – a shift to longer
wavelength ; lower energy
ii. Hypsochromic shift (blue shift) – shift to shorter
wavelength ; higher energy
iii. Hyperchromic effect – an increase in intensity.
iv. Hypochromic effect – a decrease in intensity.
 Bathochromic shift: - Absorption shifted towards longer
wavelength
- Change of solvent/ auxochrome -Red shift/ bathochromic shift
- n to * transition for carbonyl compounds experiences
bathochromic shift when the polarity of the solvent is
decreased.
 Hypsochromic shift : - Shift towards shorter wavelength
-(Blue shift) - Change of solvent towards higher polarity or
removal of conjugation
- Aniline – 280 nm (conjugation of pair of electrons of nitrogen
with benzene ring) In acidic solution it will form - NH+ 3 ,
due to the removal of conjugation or removal of lone pair of
electrons, the absorption takes place at lower wavelength
203nm.
 Hyperchromic shift: - Shift due to increase in intensity-
εmax increase - Due to the introduction of auxochrome
Ex: Pyridine - 257 nm and εmax is 2750; 2 – methyl pyridine
262 nm and εmax is 3560
 Hypochromic shift: - Inverse of hyperchromic shift
i.e., decrease of intensity - introduction of any group to the
compounds which is going to alter the molecular pattern of
the compound.
ex: biphenyl absorption is at 250 nm and 19000 εmax -
Whereas 2 –methyl biphenyl has an absorption of 237 nm and
10250 εmax
SOLVENT EFFECT
Solvent is the one in which solute is dissolved completely.
Solvent is the important factor for u.v./visible spectroscopy.
Ideal solvent :
 It should be cheaper.
 It should be easily available.
 It should be transparent & less polar Should not possess any
kind of absorption when it is exposed to radiation.
 A most suitable solvent which does not absorb the radiation.
 Most commonly used solvent is 95% ethanol, it is cheap and
is transparent down to 210m μ .
 Commercial ethanol is not used because it is having benzene
which absorbs strongly in u.v.region.
 The position as well as the intensity of absorption maximum
get shifted for particular chromophore by change in the
polarity of solvent.
 The wavelenth for the non-polar compounds is usually shifted
by change in polarity of solvent.
 α, β - unsaturated carbonyl compounds show 2 different
shifts
 n -π* transition, absorption band moves to shorter
wavelength. Due to H-bonding with solvent molecules occurs
to lesser extent with the carbonyl group in the excited state.
 E.g. A max of acetone is 279m μ in hexane, while in water
264m μ . 13
 π → π* transition, absorption band moves longer wavelength.
 The dipole-dipole interactions with the solvent molecules
lower the energy of the energy of the excited state more than
that of the ground state. Value of A max in ethanol will be
greater than that in hexane.
 П* orbital gets more stabilised by H-bonding with the polar
solvent like water & ethanol. Because of greater polarity of
П* orbital. Thus small energy is needed for transition and
absorption shows a red shift.

More Related Content

What's hot

C-13 NMR Spectroscopy
C-13 NMR SpectroscopyC-13 NMR Spectroscopy
C-13 NMR SpectroscopyMANISHSAHU106
 
Spectroflourimetry
SpectroflourimetrySpectroflourimetry
SpectroflourimetryXenChisti
 
INTERPRETATION OF MASS SPECTROSCOPY
INTERPRETATION OF MASS SPECTROSCOPYINTERPRETATION OF MASS SPECTROSCOPY
INTERPRETATION OF MASS SPECTROSCOPYvidya chowdhary
 
Interpretation of organic compounds by IR, NMR and Mass Spectrometry
Interpretation of organic compounds by IR, NMR and Mass SpectrometryInterpretation of organic compounds by IR, NMR and Mass Spectrometry
Interpretation of organic compounds by IR, NMR and Mass SpectrometryAshitoshPanchal
 
Effect of Solvent in UV-by M.Qasim.pptx
Effect of Solvent in UV-by M.Qasim.pptxEffect of Solvent in UV-by M.Qasim.pptx
Effect of Solvent in UV-by M.Qasim.pptxMEMORISEME
 
'estimation of quinine sulphate by fluorescence spectroscopy with recordings...
 'estimation of quinine sulphate by fluorescence spectroscopy with recordings... 'estimation of quinine sulphate by fluorescence spectroscopy with recordings...
'estimation of quinine sulphate by fluorescence spectroscopy with recordings...Priya Bardhan Ray
 
Quantum numbers and its roles in nmr
Quantum numbers and its roles in nmrQuantum numbers and its roles in nmr
Quantum numbers and its roles in nmrAtul Adhikari
 
Factors influencing chemical shift
Factors influencing chemical shiftFactors influencing chemical shift
Factors influencing chemical shiftKavitha Bitra
 
Absorption shifts (Chromophores and Auxophores Concept)
Absorption shifts (Chromophores and Auxophores Concept)Absorption shifts (Chromophores and Auxophores Concept)
Absorption shifts (Chromophores and Auxophores Concept)Dr Duggirala Mahendra
 
Mass Ionization Techniques
Mass Ionization TechniquesMass Ionization Techniques
Mass Ionization TechniquesMehulJain143
 
Single component analysis (uv visible spectroscopy) by mr. pradeep swarnkar
Single component analysis (uv visible spectroscopy) by mr. pradeep swarnkarSingle component analysis (uv visible spectroscopy) by mr. pradeep swarnkar
Single component analysis (uv visible spectroscopy) by mr. pradeep swarnkarPradeep Swarnkar
 
Interpretation of IR
Interpretation of IRInterpretation of IR
Interpretation of IRLokesh Patil
 
13C-NMR SPECTROSCOPY
13C-NMR SPECTROSCOPY13C-NMR SPECTROSCOPY
13C-NMR SPECTROSCOPYramanbrar09
 

What's hot (20)

C-13 NMR Spectroscopy
C-13 NMR SpectroscopyC-13 NMR Spectroscopy
C-13 NMR Spectroscopy
 
Uv absorption spectroscopy
Uv absorption spectroscopyUv absorption spectroscopy
Uv absorption spectroscopy
 
Spectroflourimetry
SpectroflourimetrySpectroflourimetry
Spectroflourimetry
 
Ir spectroscopy slide
Ir spectroscopy slideIr spectroscopy slide
Ir spectroscopy slide
 
Quenching
QuenchingQuenching
Quenching
 
INTERPRETATION OF MASS SPECTROSCOPY
INTERPRETATION OF MASS SPECTROSCOPYINTERPRETATION OF MASS SPECTROSCOPY
INTERPRETATION OF MASS SPECTROSCOPY
 
Interpretation of organic compounds by IR, NMR and Mass Spectrometry
Interpretation of organic compounds by IR, NMR and Mass SpectrometryInterpretation of organic compounds by IR, NMR and Mass Spectrometry
Interpretation of organic compounds by IR, NMR and Mass Spectrometry
 
Effect of Solvent in UV-by M.Qasim.pptx
Effect of Solvent in UV-by M.Qasim.pptxEffect of Solvent in UV-by M.Qasim.pptx
Effect of Solvent in UV-by M.Qasim.pptx
 
Mass spectrum
Mass spectrumMass spectrum
Mass spectrum
 
Quenching In Fluorimetry.
Quenching In Fluorimetry.Quenching In Fluorimetry.
Quenching In Fluorimetry.
 
'estimation of quinine sulphate by fluorescence spectroscopy with recordings...
 'estimation of quinine sulphate by fluorescence spectroscopy with recordings... 'estimation of quinine sulphate by fluorescence spectroscopy with recordings...
'estimation of quinine sulphate by fluorescence spectroscopy with recordings...
 
Ir spectroscopy
Ir spectroscopyIr spectroscopy
Ir spectroscopy
 
UV-Visible Spectroscopy.pptx
UV-Visible Spectroscopy.pptxUV-Visible Spectroscopy.pptx
UV-Visible Spectroscopy.pptx
 
Quantum numbers and its roles in nmr
Quantum numbers and its roles in nmrQuantum numbers and its roles in nmr
Quantum numbers and its roles in nmr
 
Factors influencing chemical shift
Factors influencing chemical shiftFactors influencing chemical shift
Factors influencing chemical shift
 
Absorption shifts (Chromophores and Auxophores Concept)
Absorption shifts (Chromophores and Auxophores Concept)Absorption shifts (Chromophores and Auxophores Concept)
Absorption shifts (Chromophores and Auxophores Concept)
 
Mass Ionization Techniques
Mass Ionization TechniquesMass Ionization Techniques
Mass Ionization Techniques
 
Single component analysis (uv visible spectroscopy) by mr. pradeep swarnkar
Single component analysis (uv visible spectroscopy) by mr. pradeep swarnkarSingle component analysis (uv visible spectroscopy) by mr. pradeep swarnkar
Single component analysis (uv visible spectroscopy) by mr. pradeep swarnkar
 
Interpretation of IR
Interpretation of IRInterpretation of IR
Interpretation of IR
 
13C-NMR SPECTROSCOPY
13C-NMR SPECTROSCOPY13C-NMR SPECTROSCOPY
13C-NMR SPECTROSCOPY
 

Similar to UV VISIBLE SPECTROSCOPY.pptx

UV visible spectroscopy ( electronic spectroscopy)
UV visible spectroscopy ( electronic spectroscopy)UV visible spectroscopy ( electronic spectroscopy)
UV visible spectroscopy ( electronic spectroscopy)ushaSanmugaraj
 
BASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptx
BASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptxBASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptx
BASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptxNittalVekaria
 
Uv visible spectroscopy ppt
Uv visible spectroscopy pptUv visible spectroscopy ppt
Uv visible spectroscopy pptAlexa Jacob
 
U1 C1 UV Spectroscopy.pptx
U1 C1 UV Spectroscopy.pptxU1 C1 UV Spectroscopy.pptx
U1 C1 UV Spectroscopy.pptxAnkita Raikwar
 
uvvisiblespectroscopy-130121115849-phpapp02.pptx
uvvisiblespectroscopy-130121115849-phpapp02.pptxuvvisiblespectroscopy-130121115849-phpapp02.pptx
uvvisiblespectroscopy-130121115849-phpapp02.pptxTridevSastri1
 
Uvvisiblespectroscopy 130121115849-phpapp02
Uvvisiblespectroscopy 130121115849-phpapp02Uvvisiblespectroscopy 130121115849-phpapp02
Uvvisiblespectroscopy 130121115849-phpapp02gufy ssah
 
UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]
UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]
UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]Shikha Popali
 
Uv spectroscopy
Uv spectroscopy Uv spectroscopy
Uv spectroscopy Rokon khan
 
UV visible spectroscopy.pptx
UV visible spectroscopy.pptxUV visible spectroscopy.pptx
UV visible spectroscopy.pptxJoshNobins
 
UV visible spectroscopy.pptx
UV visible spectroscopy.pptxUV visible spectroscopy.pptx
UV visible spectroscopy.pptxJoshNobins
 
uv-visiblespectroscopy final.pptx
uv-visiblespectroscopy final.pptxuv-visiblespectroscopy final.pptx
uv-visiblespectroscopy final.pptxRagisha Thomas
 
Uv visible spectroscopy
Uv visible spectroscopyUv visible spectroscopy
Uv visible spectroscopyNilesh Thakare
 
Lec.2 woodward fishers rule 13.02.17
Lec.2   woodward fishers rule 13.02.17Lec.2   woodward fishers rule 13.02.17
Lec.2 woodward fishers rule 13.02.17IBRAHIM Aminu Shehu
 
Spectroscopic methods in inorganic chemistry Part1 uv vis
Spectroscopic methods in inorganic chemistry Part1 uv visSpectroscopic methods in inorganic chemistry Part1 uv vis
Spectroscopic methods in inorganic chemistry Part1 uv visChris Sonntag
 
UV spectrometery; woodward fischer rule
UV spectrometery; woodward fischer ruleUV spectrometery; woodward fischer rule
UV spectrometery; woodward fischer ruleAJAYKUMAR4872
 
Ultraviolet and visible spectroscopy
Ultraviolet and visible spectroscopyUltraviolet and visible spectroscopy
Ultraviolet and visible spectroscopyDiksha Kataria
 
1.b. pharm uvvisiblespectroscopy jntu pharmacy
1.b. pharm uvvisiblespectroscopy jntu pharmacy1.b. pharm uvvisiblespectroscopy jntu pharmacy
1.b. pharm uvvisiblespectroscopy jntu pharmacyDr. Suman Pattanayak
 

Similar to UV VISIBLE SPECTROSCOPY.pptx (20)

UV visible spectroscopy ( electronic spectroscopy)
UV visible spectroscopy ( electronic spectroscopy)UV visible spectroscopy ( electronic spectroscopy)
UV visible spectroscopy ( electronic spectroscopy)
 
BASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptx
BASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptxBASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptx
BASIC THEORY OF UV VISIBLE SPECTROSCOPY.pptx
 
Uv visible spectroscopy ppt
Uv visible spectroscopy pptUv visible spectroscopy ppt
Uv visible spectroscopy ppt
 
U1 C1 UV Spectroscopy.pptx
U1 C1 UV Spectroscopy.pptxU1 C1 UV Spectroscopy.pptx
U1 C1 UV Spectroscopy.pptx
 
uvvisiblespectroscopy-130121115849-phpapp02.pptx
uvvisiblespectroscopy-130121115849-phpapp02.pptxuvvisiblespectroscopy-130121115849-phpapp02.pptx
uvvisiblespectroscopy-130121115849-phpapp02.pptx
 
Uvvisiblespectroscopy 130121115849-phpapp02
Uvvisiblespectroscopy 130121115849-phpapp02Uvvisiblespectroscopy 130121115849-phpapp02
Uvvisiblespectroscopy 130121115849-phpapp02
 
UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]
UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]
UV SPECTROSCOPY [ULTRA-VIOLET SPECTROSCOPY]
 
Uv spectroscopy
Uv spectroscopy Uv spectroscopy
Uv spectroscopy
 
UV visible spectroscopy.pptx
UV visible spectroscopy.pptxUV visible spectroscopy.pptx
UV visible spectroscopy.pptx
 
UV visible spectroscopy.pptx
UV visible spectroscopy.pptxUV visible spectroscopy.pptx
UV visible spectroscopy.pptx
 
uv-visiblespectroscopy final.pptx
uv-visiblespectroscopy final.pptxuv-visiblespectroscopy final.pptx
uv-visiblespectroscopy final.pptx
 
Uv visible spectroscopy
Uv visible spectroscopyUv visible spectroscopy
Uv visible spectroscopy
 
Lec.2 woodward fishers rule 13.02.17
Lec.2   woodward fishers rule 13.02.17Lec.2   woodward fishers rule 13.02.17
Lec.2 woodward fishers rule 13.02.17
 
spectroscopy sidra
spectroscopy sidraspectroscopy sidra
spectroscopy sidra
 
Spectroscopic methods in inorganic chemistry Part1 uv vis
Spectroscopic methods in inorganic chemistry Part1 uv visSpectroscopic methods in inorganic chemistry Part1 uv vis
Spectroscopic methods in inorganic chemistry Part1 uv vis
 
UV Spectroscopy
UV SpectroscopyUV Spectroscopy
UV Spectroscopy
 
UV spectrometery; woodward fischer rule
UV spectrometery; woodward fischer ruleUV spectrometery; woodward fischer rule
UV spectrometery; woodward fischer rule
 
UV Visible spectroscopy
UV Visible spectroscopyUV Visible spectroscopy
UV Visible spectroscopy
 
Ultraviolet and visible spectroscopy
Ultraviolet and visible spectroscopyUltraviolet and visible spectroscopy
Ultraviolet and visible spectroscopy
 
1.b. pharm uvvisiblespectroscopy jntu pharmacy
1.b. pharm uvvisiblespectroscopy jntu pharmacy1.b. pharm uvvisiblespectroscopy jntu pharmacy
1.b. pharm uvvisiblespectroscopy jntu pharmacy
 

Recently uploaded

Recombinant DNA technology (Immunological screening)
Recombinant DNA technology (Immunological screening)Recombinant DNA technology (Immunological screening)
Recombinant DNA technology (Immunological screening)PraveenaKalaiselvan1
 
Nanoparticles synthesis and characterization​ ​
Nanoparticles synthesis and characterization​  ​Nanoparticles synthesis and characterization​  ​
Nanoparticles synthesis and characterization​ ​kaibalyasahoo82800
 
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43bNightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43bSérgio Sacani
 
Chromatin Structure | EUCHROMATIN | HETEROCHROMATIN
Chromatin Structure | EUCHROMATIN | HETEROCHROMATINChromatin Structure | EUCHROMATIN | HETEROCHROMATIN
Chromatin Structure | EUCHROMATIN | HETEROCHROMATINsankalpkumarsahoo174
 
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...Sérgio Sacani
 
Biopesticide (2).pptx .This slides helps to know the different types of biop...
Biopesticide (2).pptx  .This slides helps to know the different types of biop...Biopesticide (2).pptx  .This slides helps to know the different types of biop...
Biopesticide (2).pptx .This slides helps to know the different types of biop...RohitNehra6
 
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
Pulmonary drug delivery system M.pharm -2nd sem P'ceuticsPulmonary drug delivery system M.pharm -2nd sem P'ceutics
Pulmonary drug delivery system M.pharm -2nd sem P'ceuticssakshisoni2385
 
Zoology 4th semester series (krishna).pdf
Zoology 4th semester series (krishna).pdfZoology 4th semester series (krishna).pdf
Zoology 4th semester series (krishna).pdfSumit Kumar yadav
 
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...Sérgio Sacani
 
Unlocking the Potential: Deep dive into ocean of Ceramic Magnets.pptx
Unlocking  the Potential: Deep dive into ocean of Ceramic Magnets.pptxUnlocking  the Potential: Deep dive into ocean of Ceramic Magnets.pptx
Unlocking the Potential: Deep dive into ocean of Ceramic Magnets.pptxanandsmhk
 
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdfPests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdfPirithiRaju
 
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsHubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsSérgio Sacani
 
Isotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on IoIsotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on IoSérgio Sacani
 
Green chemistry and Sustainable development.pptx
Green chemistry  and Sustainable development.pptxGreen chemistry  and Sustainable development.pptx
Green chemistry and Sustainable development.pptxRajatChauhan518211
 
Recombination DNA Technology (Nucleic Acid Hybridization )
Recombination DNA Technology (Nucleic Acid Hybridization )Recombination DNA Technology (Nucleic Acid Hybridization )
Recombination DNA Technology (Nucleic Acid Hybridization )aarthirajkumar25
 
Chemistry 4th semester series (krishna).pdf
Chemistry 4th semester series (krishna).pdfChemistry 4th semester series (krishna).pdf
Chemistry 4th semester series (krishna).pdfSumit Kumar yadav
 
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.Nitya salvi
 
Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...
Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...
Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...anilsa9823
 
Presentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptxPresentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptxgindu3009
 
DIFFERENCE IN BACK CROSS AND TEST CROSS
DIFFERENCE IN  BACK CROSS AND TEST CROSSDIFFERENCE IN  BACK CROSS AND TEST CROSS
DIFFERENCE IN BACK CROSS AND TEST CROSSLeenakshiTyagi
 

Recently uploaded (20)

Recombinant DNA technology (Immunological screening)
Recombinant DNA technology (Immunological screening)Recombinant DNA technology (Immunological screening)
Recombinant DNA technology (Immunological screening)
 
Nanoparticles synthesis and characterization​ ​
Nanoparticles synthesis and characterization​  ​Nanoparticles synthesis and characterization​  ​
Nanoparticles synthesis and characterization​ ​
 
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43bNightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
 
Chromatin Structure | EUCHROMATIN | HETEROCHROMATIN
Chromatin Structure | EUCHROMATIN | HETEROCHROMATINChromatin Structure | EUCHROMATIN | HETEROCHROMATIN
Chromatin Structure | EUCHROMATIN | HETEROCHROMATIN
 
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
 
Biopesticide (2).pptx .This slides helps to know the different types of biop...
Biopesticide (2).pptx  .This slides helps to know the different types of biop...Biopesticide (2).pptx  .This slides helps to know the different types of biop...
Biopesticide (2).pptx .This slides helps to know the different types of biop...
 
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
Pulmonary drug delivery system M.pharm -2nd sem P'ceuticsPulmonary drug delivery system M.pharm -2nd sem P'ceutics
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
 
Zoology 4th semester series (krishna).pdf
Zoology 4th semester series (krishna).pdfZoology 4th semester series (krishna).pdf
Zoology 4th semester series (krishna).pdf
 
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
 
Unlocking the Potential: Deep dive into ocean of Ceramic Magnets.pptx
Unlocking  the Potential: Deep dive into ocean of Ceramic Magnets.pptxUnlocking  the Potential: Deep dive into ocean of Ceramic Magnets.pptx
Unlocking the Potential: Deep dive into ocean of Ceramic Magnets.pptx
 
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdfPests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
 
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsHubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
 
Isotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on IoIsotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on Io
 
Green chemistry and Sustainable development.pptx
Green chemistry  and Sustainable development.pptxGreen chemistry  and Sustainable development.pptx
Green chemistry and Sustainable development.pptx
 
Recombination DNA Technology (Nucleic Acid Hybridization )
Recombination DNA Technology (Nucleic Acid Hybridization )Recombination DNA Technology (Nucleic Acid Hybridization )
Recombination DNA Technology (Nucleic Acid Hybridization )
 
Chemistry 4th semester series (krishna).pdf
Chemistry 4th semester series (krishna).pdfChemistry 4th semester series (krishna).pdf
Chemistry 4th semester series (krishna).pdf
 
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
 
Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...
Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...
Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...
 
Presentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptxPresentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptx
 
DIFFERENCE IN BACK CROSS AND TEST CROSS
DIFFERENCE IN  BACK CROSS AND TEST CROSSDIFFERENCE IN  BACK CROSS AND TEST CROSS
DIFFERENCE IN BACK CROSS AND TEST CROSS
 

UV VISIBLE SPECTROSCOPY.pptx

  • 2. CONTENTS:  Introduction  Electronic transitions  Chromophores  Auxochromes  Spectral shifts  Solvent effect on absorption spectra
  • 3. INTRODUCTION  Spectroscopy is the branch of science that deals with the study of interaction of electromagnetic radiation with matter.  It is the most powerful tool available for the study of atomic & molecular structure and is used in the analysis of a wide range of samples. The two main types are:  Atomic Spectroscopy; This Spectroscopy is concerned with the interaction of electromagnetic radiation with atoms which are commonly in the lowest energy state called as ground state.
  • 4.  Molecular Spectroscopy ; This Spectroscopy deals with the interaction of electromagnetic radiation with molecule.  • Electromagnetic radiation consist of discrete packets of energy which are called as photons.  • A photon consists of an oscillating electric field (E) & an oscillating magnetic field (M) which are perpendicular to each other.
  • 5.
  • 6. Wavelength (, lambda): Distance from one wave peak to the next. Units: m, cm, m, nm Frequency (, nu): Number of peaks that pass through a given point per second. Units: Cycles/second or s-1 or Hertz (Hz) Wave number Number of waves per cm.
  • 8.
  • 9. 1)σ → σ* transition.  σ electron from orbital is excited to corresponding anti-bonding orbital σ*.  The energy required is large for this transition.  e.g. Methane (CH4) has C-H bond only and can undergo σ → σ* transition and shows absorbance maxima at 125 nm. 2) π → π* transition • π electron in a bonding orbital is excited to corresponding anti- bonding orbital π*. • Compounds containing multiple bonds like alkenes, alkynes, carbonyl, nitriles, aromatic compounds, etc undergo π → π* transitions. • e.g. Alkenes generally absorb in the region 170 to 205 nm.
  • 10. 3) n → σ* transition • Saturated compounds containing atoms with lone pair of electrons like O, N, S and halogens are capable of n → σ* transition. • These transitions usually requires less energy than σ → σ* transitions. • The number of organic functional groups with n → σ* peaks in UV region is small (150 – 250 nm). 4) n → π* transition • An electron from non-bonding orbital is promoted to anti- bonding π* orbital. • Compounds containing double bond involving hetero atoms (C=O, C≡N, N=O) undergo such transitions. • n → π* transitions require minimum energy and show absorption at longer wavelength around 300 nm.
  • 11. 5) & 6) σ → π* transition & π → σ* transition .  These electronic transitions are forbidden transitions & are only theoretically possible.  Thus, n → π* & π → π* electronic transitions show absorption in region above 200 nm which is accessible to UV-visible spectrophotometer.
  • 12. CHROMOPHORES  Defined as any isolated covalently bonded group that shows a characteristic absorption of Electromagnetic radiation in the UV or visible region.  It is a Greek word. Chroma = “color” & phoros = “bearer” Compound containing chromophore is CHROMOGEN  Eg: C=C, C=O, NO2 TYPES OF CHROMOPHORES  1. INDEPENDENT CHROMOPHORES: If one chromophore is required to impart colour Eg: Azo group –N=N-, Nitroso group – NO-  2. DEPENDENT CHROMOPHORES: If more than one chromophore is required to impart colour Eg: Acetone having one ketone group is colorless whereas diacetyl having two ketone groups is yellow.
  • 13.
  • 14.  Identification of a chromophore depends on a number of factors as follows;  i) Spectrum consisting of a band near 300 mµ may contain two or three conjugated units.  ii) Absorption bands near 270-350 mµ with very low intensity εmax 10-100 are due to n → π*transitions of the carbonyl group.  iii) Simple conjugated chromophores such as dienes or α, β- unsaturated ketones have high εmax values, i.e., 10,000 to 20,000.
  • 15. AUXOCHROMES  Auxochrome: A saturated/ unsaturated group with non bonding electrons when attached to chromophore altering both wavelength as well as intensity of absorption. Eg: OH, NH2, NHR, COOH, CN, Cl etc.. Two types: 1) Basic/positive auxochromic groups Effective in acid solutions  Eg: OH, OR, NHR etc. 2) Acidic/negative auxochromic groups Effective in alkaline solutions  Eg: NO, CO, CN etc.
  • 16.
  • 18.  Substituents may have any of four effects on a chromophore : i. Bathochromic shift (red shift) – a shift to longer wavelength ; lower energy ii. Hypsochromic shift (blue shift) – shift to shorter wavelength ; higher energy iii. Hyperchromic effect – an increase in intensity. iv. Hypochromic effect – a decrease in intensity.
  • 19.
  • 20.  Bathochromic shift: - Absorption shifted towards longer wavelength - Change of solvent/ auxochrome -Red shift/ bathochromic shift - n to * transition for carbonyl compounds experiences bathochromic shift when the polarity of the solvent is decreased.  Hypsochromic shift : - Shift towards shorter wavelength -(Blue shift) - Change of solvent towards higher polarity or removal of conjugation - Aniline – 280 nm (conjugation of pair of electrons of nitrogen with benzene ring) In acidic solution it will form - NH+ 3 , due to the removal of conjugation or removal of lone pair of electrons, the absorption takes place at lower wavelength 203nm.
  • 21.  Hyperchromic shift: - Shift due to increase in intensity- εmax increase - Due to the introduction of auxochrome Ex: Pyridine - 257 nm and εmax is 2750; 2 – methyl pyridine 262 nm and εmax is 3560  Hypochromic shift: - Inverse of hyperchromic shift i.e., decrease of intensity - introduction of any group to the compounds which is going to alter the molecular pattern of the compound. ex: biphenyl absorption is at 250 nm and 19000 εmax - Whereas 2 –methyl biphenyl has an absorption of 237 nm and 10250 εmax
  • 22. SOLVENT EFFECT Solvent is the one in which solute is dissolved completely. Solvent is the important factor for u.v./visible spectroscopy. Ideal solvent :  It should be cheaper.  It should be easily available.  It should be transparent & less polar Should not possess any kind of absorption when it is exposed to radiation.  A most suitable solvent which does not absorb the radiation.  Most commonly used solvent is 95% ethanol, it is cheap and is transparent down to 210m μ .  Commercial ethanol is not used because it is having benzene which absorbs strongly in u.v.region.
  • 23.
  • 24.  The position as well as the intensity of absorption maximum get shifted for particular chromophore by change in the polarity of solvent.  The wavelenth for the non-polar compounds is usually shifted by change in polarity of solvent.  α, β - unsaturated carbonyl compounds show 2 different shifts  n -π* transition, absorption band moves to shorter wavelength. Due to H-bonding with solvent molecules occurs to lesser extent with the carbonyl group in the excited state.  E.g. A max of acetone is 279m μ in hexane, while in water 264m μ . 13
  • 25.  π → π* transition, absorption band moves longer wavelength.  The dipole-dipole interactions with the solvent molecules lower the energy of the energy of the excited state more than that of the ground state. Value of A max in ethanol will be greater than that in hexane.  П* orbital gets more stabilised by H-bonding with the polar solvent like water & ethanol. Because of greater polarity of П* orbital. Thus small energy is needed for transition and absorption shows a red shift.