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5.3.2Light and the Electromagnetic Spectrum

Radiation and Temperature Change

5 min read 5 parts Lesson 10 of 11 Unit quiz

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Section 1 of 5Absorbed and Emitted Power

5.3.2 Radiation and Temperature Change
Warming
  • If an object absorbs radiation at a higher rate than it emits, its internal energy and temperature increase.
Cooling
  • If an object emits radiation at a higher rate than it absorbs, its internal energy and temperature decrease.
Steady temperature
  • When the rates are equal, the temperature remains constant even though radiation continues to flow in and out.
Emission grows with temperature
  • As an object warms it emits more, which makes it more likely to reach a steady state.

Section 2 of 5Reaching Equilibrium

1
A cool object is placed in sunshine and begins absorbing more radiation than it emits.
2
Its temperature rises, and as it warms it emits more radiation every second.
3
The gap between absorbed and emitted power gets smaller as the temperature climbs.
4
Eventually emission equals absorption and the temperature stops rising.
5
If the incoming radiation later increases or decreases, the object settles at a new equilibrium temperature.

Section 3 of 5Surfaces and Colour

Surfaces and Colour
Matt black
  • A dull black surface is the best absorber and the best emitter of infrared radiation.
Shiny silver
  • A polished light surface reflects most radiation, so it is the poorest absorber and emitter.
Reflection
  • The radiation that is reflected does not warm the object, which is why white houses stay cooler in hot climates.
Thermos flask
  • Silvered walls reduce radiation across the vacuum gap, helping the contents keep their temperature.
SurfaceAbsorbsEmits
Matt blackVery wellVery well
Matt whiteModeratelyModerately
Shiny silverPoorlyPoorly

Section 4 of 5The Earth's Temperature

Daytime
  • The Earth absorbs radiation from the Sun, so the surface warms.
Night
  • The Earth continues to emit infrared radiation into space while receiving none from the Sun, so it cools.
Atmosphere
  • Gases such as carbon dioxide and methane absorb some of the infrared radiation leaving the surface and send part of it back.
Average temperature
  • Over a long time the average temperature stays steady only when absorbed and emitted power are balanced.
Change
  • More greenhouse gases reduce the rate of emission to space, which pushes the equilibrium temperature higher.

Section 5 of 5Exam Checklist & Tips

5.3.2 – Key Points for the Exam

  • Absorbed power The rate at which an object takes in radiation energy.
  • Emitted power The rate at which an object gives out radiation energy.
  • Equilibrium temperature The steady temperature reached when absorbed and emitted power are equal.
  • Reflector A surface that sends most incident radiation back instead of absorbing it.
  • Greenhouse gas A gas in the atmosphere that absorbs infrared radiation and re-emits some of it back to the surface.

Common Mistakes

  • Saying that the object stops radiating at equilibrium; it still emits, but the same amount that it absorbs.
  • Thinking shiny surfaces are the best emitters; they are the worst emitters.
  • Assuming the Earth's temperature stays constant because it emits no radiation at night.
  • Forgetting that darker surfaces warm up faster in sunshine because they absorb more.
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