Stellar classification

classification of stars based on their spectral characteristics
(Redirected from Spectral class)

In astronomy, stellar classification is a way of grouping stars by temperature. Star temperature can be measured by looking at its spectrum, the type of light that the star shines.

M stars are the coldest and O stars are the hottest in stellar classification. These stars are from the main sequence.

Stars are also grouped into spectral types or classes by color. In general, a star's temperature determines its color, from red to blue-white. Spectral types are named with a letter. The seven main types are M, K, G, F, A, B and O. M stars are the coldest stars and O stars are the hottest.

Harvard spectral classification

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The Harvard classification system is a one-dimensional classification scheme. Stars vary in surface temperature from about 2,000 to 40,000 kelvin. Physically, the classes indicate the temperature of the star's atmosphere and are normally listed from hottest to coldest, as is done in the following table:

Note: The conventional color description describe only the peak of the stellar spectrum. However, the actual apparent colors the eye sees are lighter than the conventional color descriptions.

Class Surface temperature[1]
(kelvin)
Conventional
color description
Actual apparent color Mass
(solar masses)
Radius
(solar radius)
Luminosity
(bolometric)
Hydrogen
lines
Fraction of all
main sequence stars[2]
O ≥ 33000 K blue blue ≥ 16 M ≥ 6.6 R ≥ 30,000 L Weak ~0.00003%
B 10000–33000 K blue white deep blue white 2.1–16 M 1.8–6.6 R 25–30,000 L Medium 0.13%
A 7500–10000 K white bluish-white 1.4–2.1 M 1.4–1.8 R 5–25 L Strong 0.6%
F 6000–7500 K yellowish-white slightly whitish 1.04–1.4 M 1.15–1.4 R 1.5–5 L Medium 3%
G 5200–6000 K yellow orangish-white 0.8–1.04 M 0.96–1.15 R 0.6–1.5 L Weak 7.6%
K 3700–5200 K orange light orange 0.45–0.8 M 0.7–0.96 R 0.08–0.6 L Very weak 12.1%
M 2500–3700 K red orange ≤ 0.45 M ≤ 0.7 R ≤ 0.08 L Very weak 76.45%

The mass, radius, and luminosity listed for each class are appropriate only for stars on the main sequence portion of their lives and so are not appropriate for red giants and blue and red supergiants. The spectral classes O through M are subdivided by Arabic numerals (0–9). For example, A0 denotes the hottest stars in the A class and A9 denotes the coolest ones. The Sun is classified as G2.

 
The Hertzsprung-Russell diagram relates stellar classification with absolute magnitude, luminosity, and surface temperature.

The Hertzsprung-Russell diagram is more often used in astronomy. It relates the absolute magnitude and the surface temperature. It is as important to astronomy as the periodic table is to chemistry.

Luminosity classes

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Luminosity classes also exist and stars can be assigned to one based on their spectrum. The conventional classes are called the Yerkes system.[3]

Yerkes luminosity classes
Class Description
0 or Ia+ Hypergiants
Ia Very bright supergiants
Iab Bright supergiants
Ib Fainter supergiants
II Bright giants
III Giant stars
IV Subgiants
V Dwarf stars (main-sequence)
VI Subdwarf stars
VII White dwarfs

Our Sun, a yellow dwarf, is G2V. Red giants are K to M and have luminosity class III. Blue supergiants are O to A with II to Ia, while red supergiants are K to M with II to Ia.

Conventional and apparent colors

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The conventional color descriptions are traditional in astronomy, and represent colors relative to the mean color of an A-class star which is considered to be white. The apparent color descriptions are what the observer would see if trying to describe the stars under a dark sky without aid to the eye, or with binoculars.[4][5]

The Sun itself is white, though it is sometimes called a yellow star. This is a natural consequence of the evolution of human optical senses: the response curve that maximizes the overall efficiency against solar illumination will by definition perceive the Sun as white, though there is some subjective variation between observers.[6]

Class O

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Type O stars are stars with temperatures of ~35,000 degrees Celsius or Kelvin. They are blue in color and can be more than 6.5 times bigger than the Sun. They are also very massive but, at the same time, very rare. Examples:

Class B

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Type B stars are blue stars which have temperatures of ~25,000 degrees (Celsius or Kelvin). They are high in helium spectral lines and luminosity (brightness compared to the Sun), with moderately strong hydrogen lines. B type stars with Balmer lines in their spectra are part of the Be stars subtype. Examples:

Class A

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Type A stars are white stars which have the strongest hydrogen lines. They are some of the brightest stars in the sky. Temperatures ~10,000 degrees Celsius or Kelvin. Examples:

Class F

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Type F stars are yellow stars that contain dominant calcium lines in their spectra. They have temperatures of ~7,500 degrees Celsius or Kelvin. Examples:

Class G

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Type G stars are yellow stars with temperatures between 5,700-6,400 degrees Kelvin. Ionized calcium and iron are present in their spectra. Examples:

Class K

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Type K stars are orange to orange-red stars with temperatures between 4,100-5,100 degrees. Molecules begin to appear in weak spectral lines. Examples:

Class M

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Type M stars are the most common type of star in the universe. Red dwarfs, smaller than the sun, temperatures 3,000-4,000 degrees Kelvin and more common than red giants, which are old 3,100 degree Celsius stars in the last stages of their life. Red hypergiants are also the biggest stars, while red dwarfs, having a fully convective structure, exhaust their hydrogen fuel very slowly compared to other stars. These stars are cool enough to allow molecules to exist intact in their atmosphere; these leave many dark spectral lines. Examples:

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References

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  1. Tables VII, VIII, Empirical bolometric corrections for the main-sequence, G.M.H.J. Habets and J.R.W. Heinze, Astronomy and Astrophysics Supplement Series 46 (November 1981), pp. 193–237, [1]. Luminosities are derived from Mbol figures, using Mbol(☉)=4.75.
  2. LeDrew G. 2001. The real starry sky. Journal of the Royal Astronomical Society of Canada. 95, 1, 32–33. [2] Note: Table 2 has an error and so this article will use 824 as the assumed correct total of main-sequence stars.
  3. "Spectral Classification". lweb.cfa.harvard.edu. Retrieved 2023-12-07.
  4. The Guinness book of astronomy facts & feats, Patrick Moore, 1992, 0-900424-76-1
  5. Charity, Mitchell. "What color are the stars?". Retrieved 2006-05-13.
  6. Andrew Hamilton. "What color is the sun?". Archived from the original on 2018-01-18. Retrieved 2012-11-15.

Other websites

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