Black-Body Radiation
- Black body radiation is the name given to the thermal radiation emitted by all bodies (objects)
- All objects, no matter what temperature, emit black body radiation in the form of electromagnetic waves
- These electromagnetic waves usually lie in the infrared region of the spectrum
- Black-body radiation can also be emitted in the form of visible light or other wavelengths, depending on the temperature
- The hotter object, the more infrared radiation it radiates in a given time
- A perfect black body is defined as:
An object that absorbs all of the radiation incident on it and does not reflect or transmit any radiation
- Since a good absorber is also a good emitter, a perfect black body would be the best possible emitter too
- As a result, an object which perfectly absorbs all radiation will be black
- This is because the colour black is what is seen when all colours from the visible light spectrum are absorbed
- The intensity and wavelength distribution of any emitted waves depends on the temperature of the body
- This is represented on a black body radiation curve
- As the temperature increases, the peak of the curve moves
- This moves to a lower wavelength and a higher intensity
Black body spectrum for objects of different temperatures
- From the electromagnetic spectrum, waves with a smaller wavelength have higher energy (e.g. UV rays, X-rays)
- When an object gets hotter, the amount of thermal radiation it emits increases
- This increases the thermal energy emitted and therefore the wavelength of the emitted radiation decreases
- At room temperature objects emit thermal radiation in the infrared region of the spectrum
- At around 1000 °C an object will emit a significant amount of red light
- At 6000 °C an object will mainly emit white or blue light (and some ultraviolet)
- At even higher temperatures objects will emit ultraviolet or even X-rays
- A black body is an object which:
- Absorbs all the radiation that falls on it, and is also a good emitter
- Does not reflect or transmit any radiation
- A black body is a theoretical object, however, stars are the best approximation there is
- The radiation emitted from a black body has a characteristic spectrum that is determined by the temperature alone
The intensity-wavelength graph shows how thermodynamic temperature links to the peak wavelength for four different bodies