Infrared Emissions & Black-Body Radiation (Oxford AQA IGCSE Physics)

Revision Note

Leander Oates

Written by: Leander Oates

Reviewed by: Caroline Carroll

Explaining Infrared Radiation Emissions

  • The particles in all substances vibrate with random thermal motion

  • This motion causes objects to emit radiation

  • The higher the temperature of the object, the faster the vibrations are, and the more infrared radiation is emitted

  • The higher the temperature of the object, the higher the frequency of the emitted infrared radiation

  • If the temperature of an object is greater than the temperature of its surroundings, the object will emit more infrared radiation than it absorbs

    • The temperature of the object will decrease as there is a net energy decrease

  • If the temperature of an object is lower than the temperature of its surroundings, the object will absorb more infrared radiation than it emits

    • The temperature of the object will increase as there is a net energy increase

  • If the temperature of the object is equal to the temperature of its surroundings, then the object will emit and absorb equal amounts of infrared radiation

    • The temperature of the object will remain constant as there is no net energy transfer into or away from the system

    • The object is in thermal equilibrium

Object in thermal equilibrium

Thermal equilibrium, for IGCSE & GCSE Physics revision notes
An object will remain at a constant temperature if its absorbs radiation at the same rate as it emits radiation

Black-Body Radiation

  • An object can reach thermal equilibrium if it is capable of emitting and absorbing radiation of every wavelength

  • Then the amount of radiation emitted and absorbed at each wavelength per second could potentially reach a point where it is equal

  • In this state of thermal equilibrium, the spectrum of wavelengths emitted depends only on temperature

  • We call this object a black-body

    • A black body is a theoretical object

    • However, stars are the best approximation

Black-body radiation curve

Black Body Curve, for IGCSE & GCSE Physics Revision Notes
Black body spectrum for objects of different temperatures
  • On a black-body radiation curve, as the temperature increases, the peak of the curve moves

  • Waves with a smaller wavelength have higher energy (e.g. UV rays, X-rays)

  • When an object gets hotter, the amount of radiation it emits increases

    • This increases the energy emitted and therefore the wavelength of the emitted radiation decreases

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Leander Oates

Author: Leander Oates

Expertise: Physics

Leander graduated with First-class honours in Science and Education from Sheffield Hallam University. She won the prestigious Lord Robert Winston Solomon Lipson Prize in recognition of her dedication to science and teaching excellence. After teaching and tutoring both science and maths students, Leander now brings this passion for helping young people reach their potential to her work at SME.

Caroline Carroll

Author: Caroline Carroll

Expertise: Physics Subject Lead

Caroline graduated from the University of Nottingham with a degree in Chemistry and Molecular Physics. She spent several years working as an Industrial Chemist in the automotive industry before retraining to teach. Caroline has over 12 years of experience teaching GCSE and A-level chemistry and physics. She is passionate about creating high-quality resources to help students achieve their full potential.