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

  1. https://www.pas.rochester.edu/~emamajek/EEM_dwarf_UBVIJHK_colors_Teff.txt
  2. https://ui.adsabs.harvard.edu/abs/2013ApJS..208....9P/abstract
  3. 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)
  4. Weidner, Carsten; Vink, Jorick S. (December 2010). "The masses, and the mass discrepancy of O-type stars". Astronomy and Astrophysics. 524