Skip to content

Course home

Sign up

5.3.2 Radiation balance and constant temperature

Constant temperature requires radiation balance

Definition

Thermal equilibrium

The condition in which an object has no net transfer of energy with its surroundings, so its temperature stays constant.

  1. An object continually absorbs electromagnetic radiation from its surroundings and emits electromagnetic radiation to its surroundings.
  2. Its temperature depends on the balance between the average power absorbed and the average power emitted.
  3. If average power absorbed is greater than average power emitted, the object's internal energy increases and its temperature rises.
  4. If average power emitted is greater than average power absorbed, the object's internal energy decreases and its temperature falls.
  5. At constant temperature, average power emitted equals average power absorbed, so the net energy transfer is zero.

Temperature changes restore the balance

  1. A warmer object emits radiation at a greater intensity than the same object when cooler.
  2. If absorption temporarily exceeds emission, the object warms and its emitted power rises until balance is restored.
  3. If emission temporarily exceeds absorption, the object cools and its emitted power falls until balance is restored.
  4. Equal powers do not mean that emission and absorption stop; both transfers continue at equal average rates.
Example

Radiation balance over one minute

  • A surface absorbs 2400 J2400\,\text{J}2400J and emits 1800 J1800\,\text{J}1800J in 60 s60\,\text{s}60s.
  • The net energy gain is 2400−1800=600 J2400-1800=600\,\text{J}2400−1800=600J.
  • The average net power is P=Et=60060=10 WP=\dfrac{E}{t}=\dfrac{600}{60}=10\,\text{W}P=tE​=60600​=10W, so the surface warms.
  • As it warms, its emitted power increases and the imbalance becomes smaller.
Common Mistake

Do not state that an object at constant temperature emits no radiation; it emits and absorbs equal average powers.

Exam technique

Use power, not a single photon

  • Compare the average rates of energy transfer when explaining whether temperature rises, falls or stays constant.
  • Write absorbed power equals emitted power for a constant temperature.
  • Use P=EtP=\dfrac{E}{t}P=tE​ when energy and time are supplied.
Self review
  • What two radiation transfers occur continuously?
  • What happens when absorbed power exceeds emitted power?
  • What condition keeps an object's temperature constant?
  • Why does emission continue at thermal equilibrium?
PreviousNext

How was this guide?

Teach Genie

Review 5.3.2 Radiation balance and constant temperature by teaching Genie

Teach it back in your own words, spot gaps, and remember it better.

Start teaching
Genie and Baby Genie

5.3.2 Radiation balance and constant temperature Revision Guide

  1. GCSE
  2. /Physics
  3. /5.3.2 Radiation balance and constant temperature

Revision notes for Edexcel GCSE Physics 5.3.2 Radiation balance and constant temperature: explanations and worked examples.

Revision guides