Stellar classification
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In astronomy, stars are classified into different types depending on their spectra; this is connected to other properties of the star such as temperature and apparent color. Currently, there are seven main types, which are in order of decreasing temperature: O, B, A, F, G, K, and M.
The classes
Class | Characteristics | Color | Temperature in K[1][2][3] | Typical mass for main sequence (M☉) |
Star samples |
---|---|---|---|---|---|
O[4] | ionized Helium (He II) | blue | 30000–50000 | >18 | Mintaka, Naos |
B | neutral Helium (He I), Balmer-Series hydrogen | blue-white | 10000–30000 | 5 | Rigel, Spica, Achernar |
A | Hydrogen, Calcium (Ca II) | white | 7500–10000 | 1,9 | Vega, Sirius, Altair |
F | Calcium (Ca II), occurrence of metals | white-yellow | 6000–7500 | 1,4 | Prokyon, Canopus, Polaris |
G | Calcium (Ca II), iron and other metals | yellow | 5300–6000 | 1,0 | Tau Ceti, Sun, Alpha Centauri A |
K | strong metal lines, later Titanium dioxide | orange | 3900–5300 | 0,7 | Arcturus, Aldebaran, Epsilon Eridani, Albireo A |
M | Titanium(II)-oxide | red-orange | 2300–3900 | 0,3 | Betelgeuse, Antares, Kapteyn's Star, Proxima Centauri |
References
- ↑ https://www.pas.rochester.edu/~emamajek/EEM_dwarf_UBVIJHK_colors_Teff.txt
- ↑ https://ui.adsabs.harvard.edu/abs/2013ApJS..208....9P/abstract
- ↑ G. M. H. J. Habets, J. R. W. Heinze: Empirical bolometric corrections for the main-sequence. In: Astronomy and Astrophysics Supplement Series. 46, November 1981, S. 193–237 (Tables VII and VIII)
- ↑ Weidner, Carsten; Vink, Jorick S. (December 2010). "The masses, and the mass discrepancy of O-type stars". Astronomy and Astrophysics. 524