Aha! Chemistry with Prof Bob
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  • 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
Module 2708
​

Why doesn’t carbon dioxide absorb the radiation coming from the sun?

Carbon dioxide molecules absorb outgoing radiation from Earth – causing warming?
​

Why, then, don’t they absorb the incoming radiation from the sun – causing cooling?
​

Why are incoming and outgoing radiations different?

Why? Let's get straight to the heart of the matter ....
​

The outgoing radiation from Earth is not the same as the incoming radiation from the sun.

The outgoing radiation has wavelengths in the infrared range, but the incoming radiation from the sun is visible light.


​Photons of infrared radiation have energy that matches the gap in the quantised energy levels of vibration of carbon dioxide molecules (Module 2706 Why do carbon dioxide molecules absorb radiations emitted from Earth). So they are absorbed.

Photons of visible light have more energy than photons of infrared light, so absorption by carbon dioxide molecules would take the vibrational energy to a level that is not “allowed”. They cannot be absorbed.

That's it. Simple! But I hear you asking yourself questions ....



​
Why is the outgoing radiation different from the incoming radiation?
​

First and foremost, the outgoing radiation is NOT (mainly) reflected radiation coming from the sun.

Picture
Commonly published representations that suggest that incoming radiation is reflected at the surface of Earth are not correct. Even use of the word “re-irradiated” can be misleading, because it implies that the emitted radiations are the very radiations that come to us from the sun.
In a state of energy balance, the amount of energy coming in is the same as the amount going out (per unit time), but the photons going out are not the very same photons that came from the sun.
​
Here is an analogy: I have a glass with water in it. I use a dropper pipette to add one drop of water. Then I use it to take out one drop of water, of exactly the same volume. And I repeat that (adding and withdrawing) many times.

The volume of water in the glass remains constant. The total volume of drops added is equal to the total volume of drops withdrawn.

But the molecules of water that have been withdrawn are not the very same molecules that were added.
​
Back to Earth's incoming and outgoing radiations, photons of the outgoing radiations are not the very photons that arrived in the incoming radiations. Even more, they do not even have the same energy (or wavelength).

​
​
Different sources of incoming and outgoing radiations

The sun emits radiations in all directions spherically. Earth’s surface receives only that relatively tiny section of the sun’s radiations that come our way.

Picture
Radiations from the sun illuminate that half of Earth which is facing the sun at that time.
If outgoing radiations were reflections of the incoming radiations, they would be emitted only from that half of Earth in daylight. That is not the case.
​

Picture
Incoming radiations are incident on half of Earth's surface, but outgoing radiations are emitted from the entire surface - where it is night as well as where it is day.
The surface of the Earth absorbs the photons of incoming radiation from the sun, and they immediately cease to exist. But their energy becomes part of Earth's energy.

Photons of outgoing radiation do not exist until the Earth emits them.

The wavelengths of incoming and outgoing radiation, and the energies of their photons, are different because their sources are different.

Earth's incoming radiation is Sun's emitted radiation. So the source of Earth's incoming radiation is the sun  The source of Earth's outgoing radiation is ..... Earth.

And the wavelengths are different because the temperature of Earth and Sun are different - a phenomenon known as black-body radiation.



​
Black body radiation

Every object emits radiation whose wavelength (or photon energy) depends only on its temperature - regardless of the material of which the object is composed.

​Regardless of composition, every object hotter than about 3000 °C is “white hot”, emitting light ranging across most of the visible spectrum.. Near 1000 °C it is “red hot”. At 10 – 50 °C, the emitted radiation is invisible to humans: it is infrared radiation.


​
Picture
This iron bar, with gradations of temperature, illustrates black-body radiation. At top right, where the temperature is about 3000 °C, the bar is white hot. In the middle, the temperature is about 1000 °C, and it is red hot. If the near end, at about 50 °C were in the dark, we would not see it because it is emitting only infrared radiation.
Outgoing radiation: 

The temperature of the surface of Earth is approximately 15 °C. Like all objects at 15 °C, Earth emits radiation whose wavelengths are in the far infrared part of the spectrum.

The photons have energy equal to the gap between the energy levels of vibration of carbon dioxide. So carbon dioxide molecules absorb the photons.


​
Incoming radiation

The temperature of the surface of the sun is 5600 °C. The sun emits mainly visible light - “white light” (wavelengths 400 – 700 nm). The energies of the photons (more or less than those of the emitted radiation?) do not match the gap between the energy levels of vibration of carbon dioxide. So carbon dioxide molecules cannot absorb the photons or the energy of the molecules would jump to a level that is not one of the "allowed" ones.


Picture
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