Aha! Chemistry with Prof Bob
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    • Table of contents
    • Index
    • TALK WITH PROF BOB?
  • LEARNING MODULES
    • Chapter 02 Stuff, matter: What is it? >
      • 0200 Stuff, matter: A theory of atoms
      • 0201 Atoms: The building blocks of all stuff
      • 0202 People classifying stuffs. Why?
    • Chapter 05 Chemical reactions, chemical equations >
      • 0500 Chemical reactions vs. chemical equations. Overview
      • 0501 Chemical amount and its unit of measurement, mole
      • 0502 The Avogadro constant: How many is that?
      • 0503 The Avogadro constant: Why is it that number?
      • 0504 Chemical formulas: What can they tell us??
      • 0505 Chemical equations: What can they tell us?
      • 0506 Limiting reactants: How much reaction can happen?
      • 0507 Balanced chemical equations: What are they?
      • 0508 Chemical reactions as competitions
    • Chapter 09 Aqueous solutions >
      • 0901 What is a solution? And what is not?
      • 0902 Miscibility of liquids in each other
      • 0903 Like dissolves like? Shades of grey
      • 0905 Dissolution of ionic salts in water: A competition
      • 0906 Can we predict solubilities of salts?
      • 0907 Solution concentration
      • 0908 Chemical species, speciation in aqueous solution
      • 0909 Solutes: Electrolytes or non-electrolytes?
      • 0910 Electrolytes - strong or weak?
      • 0911 Concentrated, dilute, strong, weak
      • 0912 Species concentration vs. solution concentration
      • 0913 Weak electrolytes: Getting quantitative
    • Chapter 11: Dynamic chemical equilibrium >
      • 1100 Dynamic chemical equilibrium: Overview
      • 1101 Visualising dynamic chemical equilibrium
      • 1102 The jargon of chemical equilibrium
      • 1103 Equilibrium constants: The law of equilibrium
      • 1104 The law of equilibrium: an analogy
    • Chapter 22 Spectroscopy >
      • 2200 Spectroscopy: Overview and preview
      • 2201 Quantisation of forms of energy
      • 2202 Light: Wave-particle "duality"
      • 2203 Ultraviolet-visible spectroscopy
      • 2204 Beer’s law: How much light is transmitted?
    • Chapter 27 The greenhouse effect, climate change >
      • 2700 The greenhouse effect: overview
      • 2701 Is Earth in energy balance?
      • 2702 CO2 in the atmosphere before 1800
      • 2703 So little CO2! Pffft?
      • 2704 Does CO2 affect Earth's energy balance?
      • 2705 The "greenhouse effect"
      • 2706 Why does CO2 absorb radiation from Earth?
      • 2707 The "enhanced greenhouse effect"
      • 2708 Why doesn't CO2 absorb the radiation from the sun?
      • 2709 Why are N2 and O2 not greenhouse gases?
      • 2710 Doesn't water vapour absorb all the IR?
      • 2711 Carbon dioxide from our cars
      • 2712 The source of energy from combustion
      • 2713 Comparing fuels as energy sources
      • 2714 Methane: How does it compare as a GHG?
      • 2715 Different sorts of pollution of the atmosphere
      • 2716 "Acidification" of seawater
    • Chapter 27 Communicating chemistry >
      • 2700 Overview, preview
      • 2703 The jargon we use
  • TEACHERS' CORNER
    • T01 Communicating chemistry
    • T02 Beer's law
    • T03 Professional amnesia of the chemistry teaching professio
    • T04 Law of equilibrium
    • T05 Visusalizing dynamic chemical equilibrium
    • Information vs. knowledge
  • PERSONAL GALLERY
    • Family
    • Travel
    • Playful dolphins
    • The University of Western Australia
    • Kings Park
    • Perth
    • At work
    • 999 Thermodynamics

Module 2200

​

Spectroscopy: Overview and preview




​Interaction of radiations and stuffs

Absorption of radiation by stuffs, emission of radiation from stuffs

​What is the nature of radiation?

Why are those particular wavelengths of radiation absobed?

Where does the energy of absorbed radiation go?
​


Picture
These bottles appear blue to us because red and yellow light have been absorbed by the glass from light coming from behind toward our eyes. Why were these particular colours absorbed, and blue and green transmitted? Where did the energy of the absorbed light go? What is light (or any form of radiation) anyway?



Overview


​Scientists can deduce evidence about the nature of matter by analysis of the particular wavelengths of electromagnetic radiation that are absorbed by materials.


Other evidence can be deduced from the particular wavelengths of radiation that are emitted by materials when subjected to high electric potential or heating - such as the colours emitted by substances in the flames in the banner image above.
​
This field of science is called spectroscopy
.

The study of the interaction of electromagnetic radiation with matter can extend from very high-energy waves (high frequencies and short wavelengths) such as gamma rays and X-rays to very low-energy waves (low frequencies and long wavelengths) such as microwaves.

These include, but go way beyond, radiation in the visible spectrum - those wavelengths which our eyes detect as coloured light from violet to red.

Interactions of matter with different regions of the total spectrum provide evidence about different aspects of the nature of matter related to, for example, the energies of electrons, the energies of vibrations of parts of molecules, and the energies of rotation (tumbling) of molecules.

These, in turn, provide evidence about the structures of atoms and molecules.
​

Spectroscopic evidence derived from the interaction of matter with all wavelengths of radiation depend upon a phenomenon way out of our daily experience: that is, that the various forms of energy of matter are quantised. This means that energy cannot be changed continuously: it can only have certain levels (and not amounts of energy in between the "allowed" levels). What an extraordinary thing to contemplate!
​

Spectra (both emission and absorption) in the visible and ultraviolet regions of electromagnetic radiation are attributed to "transitions" between "allowed" levels of energy of electrons, while spectra in the infrared region are due to "transitions" between levels of energy of vibrations in molecules. Prof Bob gives a general explanation in Module 2201: Quantization of forms of energy.

What is light: waves, particles, or neither?

Some of the properties of radiations are consistent with them being waveforms.

However, the notion that species can absorb only particular wavelengths of radiation whose energies corresponds with the differences between levels of forms of energy is only sensible if the radiation is composed of particles (“photons”).

Light is what it is: and not a waveform and a particle, nor a waveform or a particle. Because or our inability to understand the mysterious nature of light, based on our common experiences of phenomena, scientists use a “dual nature of explanations”.

Join in a conversation with Prof Bob in Module 2202: Light: Wave-particle “duality”.
​
Using a view of light as photons, Prof Bob discusses a more detailed explanation pertaining specifically to absorption of radiations in the visible and ultraviolet in Module 2203: UV-visible spectroscopy.
​
What does the fraction of light of a particular wavelength that is absorbed (or transmitted) by a coloured solution depend on? The dependence is expressed quantitatively by Beer's law (sometimes called the Beer-Lambert law).

In Module 2204: Beer's law, Prof Bob demonstrates the basis of Beer's law through a simple activity, and shows how it can be used to analyse for the concentration of a coloured component in solution.
​
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LEARNING CHEMISTRY FOR UNDERSTANDING
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  • HOME
  • NAVIGATION
    • Table of contents
    • Index
    • TALK WITH PROF BOB?
  • LEARNING MODULES
    • Chapter 02 Stuff, matter: What is it? >
      • 0200 Stuff, matter: A theory of atoms
      • 0201 Atoms: The building blocks of all stuff
      • 0202 People classifying stuffs. Why?
    • Chapter 05 Chemical reactions, chemical equations >
      • 0500 Chemical reactions vs. chemical equations. Overview
      • 0501 Chemical amount and its unit of measurement, mole
      • 0502 The Avogadro constant: How many is that?
      • 0503 The Avogadro constant: Why is it that number?
      • 0504 Chemical formulas: What can they tell us??
      • 0505 Chemical equations: What can they tell us?
      • 0506 Limiting reactants: How much reaction can happen?
      • 0507 Balanced chemical equations: What are they?
      • 0508 Chemical reactions as competitions
    • Chapter 09 Aqueous solutions >
      • 0901 What is a solution? And what is not?
      • 0902 Miscibility of liquids in each other
      • 0903 Like dissolves like? Shades of grey
      • 0905 Dissolution of ionic salts in water: A competition
      • 0906 Can we predict solubilities of salts?
      • 0907 Solution concentration
      • 0908 Chemical species, speciation in aqueous solution
      • 0909 Solutes: Electrolytes or non-electrolytes?
      • 0910 Electrolytes - strong or weak?
      • 0911 Concentrated, dilute, strong, weak
      • 0912 Species concentration vs. solution concentration
      • 0913 Weak electrolytes: Getting quantitative
    • Chapter 11: Dynamic chemical equilibrium >
      • 1100 Dynamic chemical equilibrium: Overview
      • 1101 Visualising dynamic chemical equilibrium
      • 1102 The jargon of chemical equilibrium
      • 1103 Equilibrium constants: The law of equilibrium
      • 1104 The law of equilibrium: an analogy
    • Chapter 22 Spectroscopy >
      • 2200 Spectroscopy: Overview and preview
      • 2201 Quantisation of forms of energy
      • 2202 Light: Wave-particle "duality"
      • 2203 Ultraviolet-visible spectroscopy
      • 2204 Beer’s law: How much light is transmitted?
    • Chapter 27 The greenhouse effect, climate change >
      • 2700 The greenhouse effect: overview
      • 2701 Is Earth in energy balance?
      • 2702 CO2 in the atmosphere before 1800
      • 2703 So little CO2! Pffft?
      • 2704 Does CO2 affect Earth's energy balance?
      • 2705 The "greenhouse effect"
      • 2706 Why does CO2 absorb radiation from Earth?
      • 2707 The "enhanced greenhouse effect"
      • 2708 Why doesn't CO2 absorb the radiation from the sun?
      • 2709 Why are N2 and O2 not greenhouse gases?
      • 2710 Doesn't water vapour absorb all the IR?
      • 2711 Carbon dioxide from our cars
      • 2712 The source of energy from combustion
      • 2713 Comparing fuels as energy sources
      • 2714 Methane: How does it compare as a GHG?
      • 2715 Different sorts of pollution of the atmosphere
      • 2716 "Acidification" of seawater
    • Chapter 27 Communicating chemistry >
      • 2700 Overview, preview
      • 2703 The jargon we use
  • TEACHERS' CORNER
    • T01 Communicating chemistry
    • T02 Beer's law
    • T03 Professional amnesia of the chemistry teaching professio
    • T04 Law of equilibrium
    • T05 Visusalizing dynamic chemical equilibrium
    • Information vs. knowledge
  • PERSONAL GALLERY
    • Family
    • Travel
    • Playful dolphins
    • The University of Western Australia
    • Kings Park
    • Perth
    • At work
    • 999 Thermodynamics