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