Classification of Stella Spectra

In summary, the letters O, B, A, F, G, K, and M are used to classify stars based on their spectral characteristics. This system was originally based on the darkest hydrogen spectral lines, but has since been revised to take into account effective temperature. Some mnemonics have been created to remember the order of the letters, but they do not hold any significant meaning in the classification system.
  • #1
jimmy p
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Just a simple quickie, why are stars classified using the letters O, B, A, F, G, K and M? Is there any significance in the letters?
 
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  • #2
Indeed, there is a significance. http://lheawww.gsfc.nasa.gov/users/allen/spectral_classification.html provides an overwiev
 
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  • #3
Back in the late 1800s, when Professor Draper of Harvard Observatory began his photographic collection of stellar spectra, the underlying physical significance of spectral line intensities was not understood, nor did he have a way to guess the temperatures of the stellar atmospheres that produced these spectra. But he best understood the visible Hydrogen dark lines (Balmer series) and decided to base a classification on letters of the roman alphabet: A, B, C, D,... A would be (and still is) the darkest hydrogen Balmer lines, B would be next darkest and so on down. This project was continued by Annie Cannon after Draper died. With time it became clear that the Draper system was not a particularly natural one, though thousands of records had been classified using this letter scheme. The matter of determining effective temperatures, excitation versus ionization in line spectra and their statistical distribution, and also the effects of stellar size differences on spectra led to a realization that these letters needed to be rearranged differently. For instance, O represents a hotter stellar surface condition than A, but is weak in Hydrogen lines. That is because almost all of the Hydrogen is at equilibrium in the ionized state at that temperature, so practically no Balmer lines can be detected. Most of the letters turned out to be single rare and peculiar stars, better represented by certain common letters in the system, so they were dropped. The remaining were W,O,B,A,F,G,K,M and a few others, going from hottest surface temperatures on down. The revised scheme is also complicated by existence of bright lines in the spectra of some stars.

Quart
 
  • #4
So what is the meaning of the letters?
 
  • #5
  • #6
"Oh, Be A Fine Gorilla, Kiss Me."

- Warren
 
  • #7
Just a simple quickie, why are stars classified using the letters O, B, A, F, G, K and M? Is there any significance in the letters?
Indeed, your list is not complete. It extends to 4 more classes (R,N and S by the right and W by the left)
So the list must be W O B A F G K M R N S
You can memorize it like "Wow, Oh be a fine girl, kiss me right now soon"
 
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  • #8
"girl": I understand this is no longer "PC" in certain countries in the North American continent ... and why not "guy"? or "gorilla"?

"soon": used to be "sweetheart", but also no longer PC

In any case, we now have T, L, C (?), and maybe more as classes for stars (not necessary, entirely, spectral classifications).
 
  • #9
jimmy p said:
So what is the meaning of the letters?
A bunch of memory tricks tell you nothing about the meaning of the letters. Go to:

http://www.astronomy.ohio-state.edu/~pogge/Ast162/Unit1/sptypes.html and read the progression of the classification systems all to the bottom of the page, and then click on the top or bottom link that shows comparative spectra of the different classes. The letters just happened to be rearranged as explaned on the link, and could have just as well been 1, 2, 3 etc. had letters not been originally chosen.
 
  • #10
jimmy p said:
So what is the meaning of the letters?

The meaning of the letters is that A is the first letter of the Roman alphabet, B is the second letter, C is the third letter, etc. It is a list.

The sequence was set up to begin with stars of darkest Hydrogen spectral lines first, next darkest second, and so on. Most of the classes (letters) were later thought unnecessary. Effective temperature became more physically important than the original idea of Hydrogen dark lines. So the remaining classes (letters) got their order changed to go from highest effective emission temperature on down.
 
  • #11
chroot said:
"Oh, Be A Fine Gorilla, Kiss Me."

- Warren

oh yeh! no prob u lady gorilla u! pphhwwaa!
 
  • #12
jimmy p said:
just a simple quickie, why are stars classified using the letters o, b, a, f, g, k and m? Is there any significance in the letters?

legend jimmy p! {:-)
 

1. What is the purpose of classifying Stella Spectra?

The purpose of classifying Stella Spectra is to organize and categorize the different types of stars based on their spectral characteristics. This allows scientists to better understand the evolution and properties of stars, as well as their place in the universe.

2. How are Stella Spectra classified?

Stella Spectra are classified using the Harvard spectral classification system, which is based on the presence and intensity of certain spectral lines in a star's spectrum. This results in a single-letter spectral type, from hottest to coolest: O, B, A, F, G, K, and M.

3. What factors determine the spectral type of a star?

The spectral type of a star is determined by its temperature, which affects the types of atoms and molecules present in its atmosphere. Cooler stars have more molecules, leading to the presence of more spectral lines, and thus a different spectral type.

4. How does the spectral type of a star relate to its color?

The spectral type of a star is directly related to its color, with hotter stars appearing bluer and cooler stars appearing redder. This is due to the fact that the temperature of a star affects the types of light it emits, with hotter stars emitting more high-energy, shorter-wavelength light (blue) and cooler stars emitting more low-energy, longer-wavelength light (red).

5. What other information can be gleaned from Stella Spectra classification?

In addition to determining the spectral type and color of a star, classification of Stella Spectra can also provide information about a star's composition, age, and even its distance from Earth. This can help scientists better understand the formation and evolution of stars, as well as their role in the larger universe.

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