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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!

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16y ago

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