ROY G BIV

May 27th, 2008

My mother is reading Spider Star and liking it significantly more than Star Dragon, primarily because she feels more for the characters.   She hasn’t finished the book yet, but did tell me on the phone the other day that she’d noticed an error.   Not a typo, but an outright mistake.

She claimed I’d gotten the temperature sequence of the colors of the rainbow incorrect.   The mnemonic “ROY G BIV” describes the sequence, running from red through orange, yellow, green, blue, indigo, and violet.

She was wrong, but it was a reminder for me about communicating science that is second nature to me and how easy it is to forget the general audience.     Let’s talk about the specific instance in Spider Star.   It’s in regard to the color of stars, and their temperatures, as they evolve.   Hotter stars are bluer, while cooler stars are redder.

To most people, red is a warm color, while blue is a cool color.   Warm stoves glow red, after all, and icy things and cool water look blue or bluish.   Artists think this way, very much, as do those in fashion and decorating.   But this is completely backwards to an astrophysicist.

Blue photons have higher frequencies and energies than red photons.   When you heat a dense gas, as in the atmosphere of a star, it does warm up and glow red.   If you continue to increase the temperature, the gas will put off a higher fraction of higher energy photons.   At some point it will be “white hot” when it’s emitting a lot of visible light at all wavelengths (remember color wheels and how mixing all the colors gives you white).   Continuing to heat the gas will give you a blue tint.

An aside: these points also explain why there are no green stars.   When you heat something to a temperature such that the peak photon energies correspond to green light, intermediate between red and blue energies, there is enough light at all visible wavelengths that the star will appear white.   With good eyes/telescopes, you can see stars in the sky that appear red, white, and blue, but never green.

The technical term for how hot dense gases, solids, and liquids radiate as a function of temperature is blackbody radiation, although I always hated the term because radiating objects sure don’t look black, do they?   Anyway, the wiki link just above goes into more detail for those interested, plotting actual spectra.

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