1/16
Looks like no tags are added yet.
Name | Mastery | Learn | Test | Matching | Spaced | Call with Kai |
|---|
No analytics yet
Send a link to your students to track their progress
Spectroscopy
Study of the production, measurement and interpretation of spectra arising from the interaction of electromagnetic radiation [EMR] with matter
Types of spectroscopy
Ultraviolet (UV)
Visible (Vis)
Infrared (IR)
Atomic Absorption
Atomic Emission
Ramen
Electromagnetic Radiation (EMR)
Particles of energy that move through space with wave-like properties
Travels through space (vacuum) at the speed of light
Described by:
𝝀 = wavelength (nm)
𝝂 = frequency (1/time)
Wavelength (𝝀)
Distance between 2 consecutive crests (peaks) on any given wave
𝝀*𝝂 = c (c= 2.99792 × 108 m/s)
Frequency (𝝂)
Number of oscillations per second (Hz = 1/s)
Determined by the source of radiation (light) and it remains constant as EMR travels through space and different media
𝝀*𝝂 = c (c= 2.99792 × 108 m/s)
Amplitude (A)
Height of the wave
Particle theory of light
Light can also be described as particles of energy that move through space with wavelike properties
Photons
Energy of a photon is quantized; it exists in discrete steps
Energy of a photon (E) is equal to the frequency of the wave (𝝂) x Planck’s constant (h = 6.6262 × 10-34 J/sec)
E = h𝝂
Photons with a higher frequency will have more energy
Quantized energy states of atoms and molecules
Energy of atoms and molecules is not continuous but exists in discrete steps (quanta)
Under normal conditions atoms & molecules exist in the lowest energy state (ground state)
Energy can be absorbed by atoms and molecules and they can be elevated to higher energy levels
The potential energy of an atom and molecule will correspond to the energy differences between excited and the ground state
Electronic energy states of an atom
When the electron relaxes to ground state, light is emitted as a photon with a wavelength that is associated with that specific energy transition
UV-Vis Spectroscopy
Involves EMR between ~100-780 nm
UV from 100-400 nm (colorless)
Visible range from 400-780 nm
Types:
Absorption spectroscopy
Emission spectroscopy
Fluorescence spectroscopy
Types of UV-Vis Measurements
Qualitative - molecular identification based upon the whole absorbance spectrum (fingerprint)
Identification is done by comparing the absorption spectrum with the spectra of a known standard compound
Quantitative (measuring) - determining the exact concentration of an analyte
Requires a standard (Beer’s law)
measurement of the amount of light absorbed as it passes through a sample solution
Principles of UV-Vis Spectroscopy
Absorption of EMR by a molecule causes electrons to move from ground to excited states
Absorption is restricted to certain functional groups: CHROMOPHORES - contain valence electrons of low excitation energy that can absorb energy in the UV-Vis range
SHORTER 𝝀 = more energy
Molar Absorptivity (ε)
Measurement of how strongly chromophores absorb light at a given wavelength
Think double bonds
Spectrophotometer Components
Light source
Emits a continuous band of EMR encompassing a wide range of ERM
Monochromator (monochromatic light)
Isolates the specific 𝝀max to be measured
Sample cell/reference cell
Detector
Converts the light transmitted through the sample cell (photons) into an electric signal
Computer
Fluorescence Spectroscopy
3 step process that describes the absorption and emission of ERM by certain highly conjugated molecules
Fluorophore: a molecule that upon absorption of EMR will emit a photon of a lower energy (longer 𝝀)
HIGHLY SENSITIVE technique
More sensitive than UV
Very selective technique because there 2 𝝀 of light involved:
Excitation wavelength
Emission wavelength
Excitation
A photon of energy is supplied by an external source (lamp) and is absorbed by the fluorophore, creating an excited electronic state
Excited state
Exists for a finite time (quick)
Fluorophore undergoes conformational changes and part of its energy is dissipated
Emission
Photon of energy is emitted, returning the fluorophore to its ground state
Due to energy dissipation during the excited-state lifetime, the energy of this photon is lower and the 𝝀 light emitted is longer