Blue Light from a Blackbody Radiator

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Discussion Overview

The discussion revolves around the emission of blue light from blackbody radiators, particularly in relation to Wien's law and the temperatures required to produce such light. Participants explore whether blue light can be predominantly produced through heating a blackbody and the mechanisms behind the perception of blue and ultraviolet light.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants note that Wien's law indicates a temperature of approximately 6500K is needed for a blackbody to emit predominantly blue light, questioning the mechanisms behind the observed blue light and ultraviolet radiation.
  • Others argue that Wien's law describes only the peak of the blackbody spectrum and that blackbodies emit wavelengths both above and below this peak.
  • One participant inquires whether it is possible to heat a blackbody to achieve mostly blue radiation, suggesting ambiguity in the term "blue."
  • Another participant points out that while a blackbody may peak in the ultraviolet range, the human eye's sensitivity to light below 450nm affects the perceived color, leading to a brilliant blue appearance instead of violet.
  • References to stellar classification are made, indicating that blackbodies above 10,000K appear blue-white to blue, with specific stars like Rigel and Vega noted as examples.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between temperature and the perception of blue light from blackbodies, with no consensus on whether a blackbody can be heated to predominantly emit blue radiation.

Contextual Notes

There are limitations in the discussion regarding the definitions of color perception and the assumptions about human sensitivity to different wavelengths of light. The relationship between temperature and color emission remains unresolved.

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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