| Region |
Wavelength |
Relative size |
Source |
| Gamma Rays |
< 0.01nm (10-12) |
Atomic Nuclei |
Nuclear reactions in objects which are highly dense and energetic such as Black Hole |
| X-rays |
0.01 - 10nm (10-8 - 10-12) |
Atom |
Super-heated gas from exploding stars when temperatures are near millions of degrees |
| Ultraviolet |
10 - 310nm |
Molecules |
Young hot stars |
| Visible |
400 - 700nm |
Bacteria |
Sun |
| Infra-Red |
710nm - 1�m |
Viruses |
Our bodies radiate with peek intensity of about 900nm at 37�C |
| Microwaves |
1�m - 1mm |
sugar grain |
Mobile phones, microwave ovens |
| Radio |
> 1mm |
FM: 1m AM: Xm |
Radio waves are found everywhere, most notably in background radiation of universe. Radio stations send electromagnetic radiation (radio waves) in patterns to our radio which in turn decodes this pattern and translates it to sound. |
Note:
- Number of waves that pass through a point in one second is called Frequency (measured in Hertz)
- Wavelength is inversely proportional to the frequency; as wavelength decreases, frequency increases
- v = l x n where:
- v = velocity of wave
- l = wavelength
- n = frequency
- Energy is directly proportional to the frequency of light; as frequency increases, energy emission increases
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