This question has a real subtlety in it.
The simplest answer is given by Wein's Law, sometimes called Wein's Displacement
Law:
The peak of the spectrum for any "blackbody" (this works approximately for
stars and people, basically any opaque object).
Wavelength of peak emission = (Stefan's constant, which you can look up) x 0.0029meter / temperature in Kelvins.
According to this formula, the peak is in the green part of the spectrum.
But a lot of light is given off across the visual part of the spectrum so it looks
whitish to me.
Here's the subtlety that few people realize. This all works only when you plot
the spectrum as the emission per unit wavelength. You can also plot the emission
per unit frequency. Then the peak is at a different location!
In the Sun's radiation, the peak intensity comes in the yellow part of the spectrum.
that depends on the wavelength of the radiation. the shorter the wavelength the more damage it can do.
the smallest infrared radiation wavelength is ranging from 0.75-1.3micrometre
No, gamma rays have the shortest wavelength.
Gamma radiation
The color of a star is related with the wavelength of the light observed. Wien's Law states that: Peak Wavelength x Surface Temperature = 2.898x10-3 Peak Wavelength is the wavelength of the highest intensity light coming from a star.
The peak wavelength, is connected to the temperature of the objects. we have short peak wavelength when the temperature is high.
The wavelength.
The wavelength.
you label a wavelength with amplitude, wavelength, through, and peak.
Infrared radiation is long wavelength radiation given out by stars.
the four parts of a wavelength are the peak, trough, wavelength, and the amplitude.
The distance from on peak to the next peak
that depends on the wavelength of the radiation. the shorter the wavelength the more damage it can do.
the smallest infrared radiation wavelength is ranging from 0.75-1.3micrometre
X rays have a wavelength of 4.2 nm.
The wavelength is inversely proportional to its frequency. That is, as the frequency increases, the wavelength decreases and vice versa.
The peak-to-peak amplitude is the distance from the trough to the crest. The wavelength is the distance from one crest to the next crest.