Oh, Be A Fine Girl, Kiss Me, Less Tongue, Yo

The constellation Orion, with Rigel, Betelgeuse, and Mintaka labeled.

Every student in introductory astronomy learns the mnemonic “Oh Be a Fine Girl/Guy, Kiss Me”, which is a way to remember the spectral classification of stars. Here’s how it works: the color of a star is determined by its temperature, as I outlined previously.

  • Oh: O class stars are the hottest, with peak temperatures in the ultraviolet part of the spectrum. They have a blue tinge to our eyes; a prime example of an O star is Mintaka, one of the stars in the “belt” of Orion.
  • Be: B class stars come next, still appearing bluish to us. Rigel, the brightest star in Orion, is a B class star — one you can see and identify easily.
  • A: A class stars are white-hot; Sirius the Dog Star, the brightest star in the night sky, falls into this category. (Harry Potter fans who are astronomy buffs were unsurprised to learn that Sirius Black could turn into a black dog for that reason.)
  • Fine: F stars are also white-hot, though with a yellow tinge. Polaris, the North Star, is F class.
  • Guy/Girl (whichever your preference): G stars are like our Sun: white, but with a yellower tinge than F stars.
  • Kiss: K stars like Arcturus in the wonderfully-named constellation Boötes  are fading towards the red part of the spectrum, and finally
  • Me: M stars such as Betelgeuse are very red in appearance. Most stars in the universe are M-type.

We teach this mnemonic (or one like it) because the letters are obviously not in alphabetical order. As with many things, the scheme is historical: originally the spectral classification was based on the absorption of light by atoms in the star’s atmosphere. Class A stars have the strongest hydrogen absorption, class B stars come next, etc. Harvard astronomer Annie Jump Cannon (who has one of my favorite names in astronomy) clarified and refined the system in the early 20th century.

Anything warm produces light; stars are special because their heat comes from nuclear fusion deep below the surface. Brown dwarfs are star-like objects that aren’t massive enough to generate nuclear fusion, but are larger and intrinsically warmer than gas giant planets like Jupiter. (I say “intrinsically”, because many exoplanets fall into the category of “hot Jupiters”: Jupiter-like worlds that orbit very close to their host star and as a result get really heated up. Jupiter’s cloud tops are quite cold, though its interior is hot.) Some brown dwarfs are warm enough to be class M, but others produce too little visible light and fall into additional categories L and T, so that I often refer to them as MLT or  “mutton, lettuce, and tomato” objects.  With L and T added, the mnemonic gets extended to “Oh, Be A Fine Guy/Girl, Kiss Me, Less Tongue” (or talk, if your professor is more squeamish).

Infrared image of a brown dwarf with a surface temperature of roughly 80 degrees Fahrenheit.

Yesterday, NASA astronomers working on the Wide-field Infrared Survey Explorer (WISE) announced the discovery of six brown dwarfs that are even less cooler than T class. These brown dwarfs have room-temperature surfaces — still warmer than Jupiter, but by far the coldest star-like objects ever observed. Humans have warmer skins than these objects, although because they are a lot bigger than us (insert a “yo momma” joke here), there’s a lot more surface area to make the light. As you can imagine, they aren’t that easy to detect, which is why it takes a highly sensitive instrument like WISE to find them, even if they are relatively close to our Solar System.

Being cooler than T class, the new brown dwarfs have been given a new spectral class Y, which astronomy teachers will have to tack on the end of the mnemonic. I don’t think the title to this post will catch on, so leave your own suggestions in the comments!

9 responses to “Oh, Be A Fine Girl, Kiss Me, Less Tongue, Yo”

  1. In the old days, say 50 years ago, spectral classes ‘R’ and ‘N’ were commonly used. I have forgotten what kind of stars they were. But this meant that the mnemonic included them, tacked onto the back end. So, what we memorized in those days was: “Oh Be A Fine Girl, Kiss Me Right Now”. Note that in those days we were not gender-neutral — we didn’t start doing that until at least a decade later.

    1. Based on where they fall, it would have to be brown dwarfs like L and T, unless M used to be subdivided.

      It’s ironic to be male-centric in this particular mnemonic, when the originators of the spectral classification were women (Annie Jump Cannon, refining a rather baroque scheme by Antonia Maury).

      1. @Mathew, I’m happy to report that my text book is sex-neutral. Here’s how it’s written in my textbook: “Oh Be A Fine Girl/Guy, Kiss Me.”

  2. […] interstellar regions. Some also may have formed as single objects, but being even smaller than brown dwarfs won’t emit even the tiny amount of infrared those weird things […]

  3. […] not right next door, but both close and luminous enough that it can be seen without a telescope. It’s an A class star, so it’s significantly hotter than the Sun; but it’s also a lot younger, possibly only a few hundred million years old, compared to our […]

  4. […] in both women’s and men’s sizes. Whoever you like kissing, I have the shirt for you. (I have more information about Cannon and the motto on the shirts here.) Advertisement Eco World Content From Across The Internet. Featured on EcoPressed Clothing […]

  5. […] earlier posts on the subject, the color of a star is dictated by its surface temperature. Hot stars appear blue or blue-white, while cool stars appear red. However, no matter how hot or cool the star, it produces a lot of […]

  6. […] the mass of the Sun, and far hotter, having a blue color. (For those keeping track at home, its spectral class is O.) What brings ζ Oph to our attention today, however, is its […]

  7. […] white, yellow, and orange, but no green. (For more on star colors and how they are classified, see my earlier post “Oh be a fine girl, kiss me, less tongue, yo“.) How humans perceive the color of stars is as much a matter of physiology and psychology as […]

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