Aha! Chemistry with Prof Bob
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  • 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 2201

Quantisation of forms of energy

Why do 'excited' hydrogen atoms emit radiation of only particular energies? How do we explain line emission spectra?

Why in the visible and ultraviolet parts of the spectrum?

Electrons in atoms can only have particular amounts of energy!?

Why are absorption or emission spectra due to change of quantised vibrational levels in the infrared region?

Why are spectra due to change of energy levels of rotation of molecules in the microwave region?
​

Tune in to Prof Bob .......
Wondrous stuff, you have to agree? Is your own personal energy quantised?
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KEY IDEAS - Quantisation of forms of energy

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This runner seems to be abled to run at any speed at all. No discontinuities. Or are the energy levels very close together for macro objects? Is your speed quantised?

The electromagnetic spectrum: The full range of wavelengths of radiation


​I refer to various regions of the electromagnetic spectrum, so let’s understand what these various regions are.
​
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The artificially proscribed regions of the electromagnetic spectrum, and the names commonly used for them.
Source: NOAA (National Oceanic and Atmospheric Administration) https://www.esrl.noaa.gov/gmd/outreach/info_activities/pdfs/TBI_electromagnetic_radiation.pdf

​
Waves range from the long-wavelength (low-frequency) radio waves to the short-wavelength (high-frequency) gamma rays. An alternative conception of radiation is as particles, or “quanta”. The quanta corresponding with radio waves are low-energy particles, and those corresponding with gamma rays have high energy.

'White light'


“White light” can be shown (by diffraction through a prism) to consist of all of the colours of the rainbow; that is, all of the wavelengths (or frequencies, or quantum energies) of radiation that we see as colours.
​
Picture
White light can be shown to consist of radiations with a range of wavelengths (or frequencies, or colours, or quantum energies.)
Image credit: https://www.weather.gov/jetstream/color

The evidence: Line emission spectrum of 'excited' atoms at visible and ultraviolet frequencies


​In contrast to white light, the radiation emitted by a sample consisting of hydrogen atoms (at high temperature, or subjected to a high electrode potential) has only particular wavelengths: there are no radiations emitted with wavelengths other than these.

​
The emission spectrum from other substances existing as atoms, and that have been “excited” by heat or electric potential, are similar to that of atomic hydrogen, although the particular wavelengths emitted are different. Hydrogen atoms have only one electron: all other atoms have more than one.
​
Picture
On top is the continuous spectrum of “white light” emitted by the sun. Below are the line spectra emitted by “excited” (energised) sodium, hydrogen and calcium atoms, respectively. How can it be that radiations are emitted at particular wavelengths, but at none of the wavelengths in between?
How to explain? Can you imagine the arousal of curiosity among chemists of the day!?

​

An explanatory model: quantisation of energy


​Niels Bohr provided a level of explanation that involved an idea that is as extraordinary now as it was then: that the electron in each hydrogen atom can only have particular energies. This is called quantisation of the electron’s energy.

Bohr’s proposition, now commonly accepted was that emission spectra arise from the energy of the electron falling from one “allowed” energy level to a lower one. A quantum of radiation is emitted whose energy is that of the difference between the upper and lower “allowed levels.

This energy of the emitted quantum (which can be regarded as a waveform of particular frequency and wavelength) is one of the lines detected in the spectrum.

A number of “de-excitations” are possible (such as level 2 down to level 1, level 3 to level 1, level 3 to level 2, …….), and for each one, a quantum of particular energy, equal to the difference between the energies of the upper and lower levels) is emitted. Each gives rise to a line in the emission spectrum.

It happens that the differences between the energy levels of electrons are such that the energy of the emitted quanta correspond with the visible region (those which our eyes can detect) and more energetic (ultraviolet radiation).



Absorption spectra
​

Absorption spectra are the opposite of emission spectra. When “white light” is passed through atomic substances, radiations of only certain wavelengths are absorbed.
​
These absorption spectra are entirely consistent with the notion of quantisation of the energies of electrons: the electrons can only be “excited” from one “allowed” energy level to another “allowed” energy level. And the energy difference of the jumps corresponds exactly with the energies of the quanta absorbed to allow the jump to happen.


​

Spectroscopy in the infrared range: vibrational energy quantised


Molecular substances also absorb particular wavelengths of radiation in the infrared range. Atomic substances do not absorb these radiations of longer wavelength (or lower frequency, or lesser quantum energy) than the visible range. How can this phenomenon be explained?

As well as the energy of the electrons, molecules have a form of energy that atoms cannot have: energy of vibrations. And the energy of each vibrational mode of a molecule (such as stretching, or bending) is quantised: that is, only certain energy levels are possible (we say “allowed”).

So the only energies that are absorbed from radiations passed through a molecular substance are those that correspond with the energy differences between levels.

“Allowed” energy levels of vibration of molecules are closer than the “allowed” energy levels of electrons in atoms, so the energies of quanta of radiation absorbed due to vibrational “excitation” are smaller than those due to electronic excitation.
​
It happens that the gaps between vibrational energy levels are such that the absorbed quanta have energies in the infrared region. 
Picture
Absorption spectrum of carbon dioxide in the infrared range, showing the specific wavelengths at which radiation is absorbed. The various modes of quantised vibrational levels responsible for the various ranges of absorption are indicated. Wavenumber is a measure of wave frequency: the higher the number, the lower is the frequency.
Source: NOAA (National Oceanic and Atmospheric Administration)
We see bands of absorption, rather than lines, because there may be several modes of vibration (symmetric stretching, antisymmetic stretching, bending) and for each one, there may be excitations between “allowed” vibrational energy levels of different electronic energy levels.

Analysis of the absorption spectra of molecular compounds allows chemists to deduce much information about the structures of their molecules – particularly to allow immediate recognition of the presence of specific functional groups (such as the alcohol –OH group, the carboxylic acid –COOH group, or the aldehyde –CHO group).

The particular ranges of infrared radiation that carbon dioxide absorbs is the reason that it is an important “greenhouse gas” affecting global climate.

​

Spectroscopy in the microwave range: quantised rotational energies


​Molecular substances also absorb radiations in the long-wavelength (low frequency, low quantum energy) region of the spectrum known as the microwave region. This is attributed to quantization of the energy of rotation (tumbling action) of the molecules.

“Allowed” rotational energy levels are even closer than
 vibrational energy levels. So the differences between levels are smaller, and the energies of absorbed quanta (equal to the differences between energy levels) are smaller. The corresponding wavelengths of the radiations are in the microwave region.

Microwave absorption spectra have been a valuable source information about the structure of molecules.
​
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SELF CHECK - Some thinking tasks

Picture
Radiation from an excited hydrogen atom that is passed through the slits of a diffraction grating can be seen to have only particular energies. The particular emitted energies do NOT correspond the 'allowed' energy levels of the electron in hydrogen atoms. Rather, they correspond with the GAPS between the energy levels. Got it? Test yourself.
Picture
Picture
Picture
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Answers

1.     (i)  Quanta emitted can have 2, 3, 4, 5, 7, or 9 units of energy.
       (ii)  
Quanta absorbed can have 2, 3, 4, 5, 7, or 9 units of energy.

2.   (c)
3.   (d)
4.   (a)


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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