Blue Light from a Blackbody Radiator

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SUMMARY

The discussion centers on the characteristics of blue light emitted by blackbody radiators, specifically referencing Wien's Law. It is established that a temperature of approximately 6500K is required for a blackbody to emit blue light, but blackbodies can emit light across a spectrum, including ultraviolet (UV) wavelengths. The perception of blue light is influenced by human eye sensitivity, which diminishes below 450nm, leading to the appearance of blue rather than violet in high-temperature blackbodies. Notable examples of bluish stars include Rigel and Vega, which exhibit their color more vividly through optical aids.

PREREQUISITES
  • Understanding of Wien's Law and its application to blackbody radiation
  • Knowledge of the electromagnetic spectrum, particularly UV and visible light
  • Familiarity with human visual perception and color sensitivity
  • Basic astronomy, including stellar classification and characteristics of stars
NEXT STEPS
  • Research the implications of Wien's Law on blackbody radiation at various temperatures
  • Explore the electromagnetic spectrum, focusing on UV and visible light wavelengths
  • Study human visual perception, particularly the sensitivity of rods and cones in low light
  • Investigate stellar classification and characteristics of blue stars like Rigel and Vega
USEFUL FOR

Astronomy enthusiasts, physicists, and anyone interested in the properties of light and color perception in relation to blackbody radiation.

Arup Biswas
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From Wien's law it is seen that approx 6500K(Greater than sun's temp) needed to heat a body to blue! But we see so much blue light(uv ray)! Are they formed from any different mechanism rather than heating?
 
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Arup Biswas said:
From Wien's law it is seen that approx 6500K(Greater than sun's temp) needed to heat a body to blue! But we see so much blue light(uv ray)! Are they formed from any different mechanism rather than heating?
Wein's law just describes the peak of the black body spectrum. A black body produces wavelengths both above and below the peak wavelength.
 
My point is can we heat a blackbody to get mostly Blue radiation??
 
Arup Biswas said:
My point is can we heat a blackbody to get mostly Blue radiation??
Yes and no.

From my research this morning, "Blue" is kind of a laymanishy term.

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You'll pretty much never see a blackbody that appears violet though, since the eye's sensitivity drops so much below 450nm that even a blackbody that peaks in the UV will appear to be a brilliant blue. There's a chart on the wikipedia article about stellar classification (https://en.wikipedia.org/wiki/Stellar_classification), but basically any blackbody over about 10,000K will appear blue-white to blue. There are several stars visible to the naked eye that are fairly bluish (Rigel and Vega spring to mind), but you'll get a much stronger color impression if you look at them through binoculars or a telescope, since dim light doesn't tend to provide much color (the rods in your eye are much more sensitive than the cones, but they do not convey color information).
 

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