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

Revision Note

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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