Understanding Starlight: White Light, Double Slit Experiment, and Color Emission

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SUMMARY

This discussion clarifies the nature of light emitted by stars, particularly focusing on the Sun and its classification as a white light source. All stars emit light across a spectrum of wavelengths, with the intensity and peak frequency of this light determined by their surface temperature. For instance, a star with a surface temperature of 15,000 Kelvin appears blue due to a higher fraction of blue wavelengths in its spectrum. The perception of the Sun as white light is influenced by human biology and evolutionary factors, making color perception subjective.

PREREQUISITES
  • Understanding of thermal radiation principles
  • Familiarity with the concept of star classification based on temperature
  • Basic knowledge of light wavelengths and their properties
  • Awareness of human color perception and its biological basis
NEXT STEPS
  • Research the relationship between star temperature and color emission
  • Explore the concept of blackbody radiation and its application to stars
  • Study the effects of human biology on color perception in different lighting conditions
  • Investigate the spectral analysis techniques used to determine star temperatures
USEFUL FOR

Astronomy enthusiasts, physics students, educators, and anyone interested in the properties of light and color perception in relation to stellar phenomena.

Zack K
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I've been recently watching videos about white light and the double slit experiment and how it creates a rainbow. It let me to some confusion and I would like some clarification.
My questions are: Do all stars like ours produce white light? Would red giants only emit red light and blue giants only emit blue light? Why does our sun produce white light and not all the types of visible light separately?
Some clarification would be amazing.
 
Science news on Phys.org
These might help:
http://csep10.phys.utk.edu/astr162/lect/light/spic-sun-ant.gif
BB_Spectra.jpg
 
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The basic reason stars emit light in the first place is because they are hot. Both the intensity and peak frequency increase with increasing temperature. Hotter stars emit more light and the intensity of that light peaks at a higher frequency than cooler stars. Note that in the top graph in Dave's post, the intensity has been normalized, meaning that each star's graph is scaled so that they peak at the same vertical distance. Spica actually puts out MUCH more light than the Sun does at all frequencies, as the bottom graph shows.

See this article: https://en.wikipedia.org/wiki/Thermal_radiation
 
So is the first graph indicating that our sun emits light from all types of wavelengths because of it's temperature?
 
Zack K said:
So is the first graph indicating that our sun emits light from all types of wavelengths because of it's temperature?
All stars emit light in all "types" of wavelengths

It so happens that the sun emits light with a quite even distribution among the so called visible wavelengths.

A star with surface temperature of 15 000 Kelvin will appear blue to us, because its spectrum contains a much larger fraction of blue wavelengths.

In fact, when one studies stars, the opposite is done. One obtains a spectrum and thus calculate the temperature of the star

(white light is also a biological effect, we think the sun is white because our eyes and brains have evolved on earth... the concept of color is subjective)
 
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malawi_glenn said:
(white light is also a biological effect, we think the sun is white because our eyes and brains have evolved on earth... the concept of color is subjective)
We are very subjective and a 'white' or grey surface will look white or grey to us under many different lighting conditions. It's quite amazing really. We can be looking at a 'red' sunset and things may have a reddish tinge to them but we can still recognise a grey as grey. Or brain is working overtime to be as consistent as possible with our colour perception. A vital evolutionary advantage (obviously).
 

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