G K M Type Stars
The nomenclature is rooted in long obsolete ideas about stellar evolution but the terminology remains. Intermediate mass stars ie spectral type a may be radiative throughout.
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A red dwarf is a small cool very faint main sequence star whose surface temperature is under about 4000 k.
G k m type stars. More discussion on the internal structure of main sequence stars is available from nasas goddard space flight center nearby k stars by distance. By comparison low mass stars sol type f g k and cooler stars have convective outer layers and radiative cores. Red dwarfs are the most common type of star.
O b and a type stars are often referred to as early spectral types while cool stars g k and m are known as late type stars. The temperature of each spectral class is then further subdivided from hot to cool by the simple addition of a number where 0 is the hottest and 9 the coolest. For supergiant stars the surface temperature range for spectral type g is host to the yellow evolutionary void where supergiant stars often swing between o or b blue and k or m red but do not stay for very long as a g star because this is an extremely unstable temperature range for supergiants.
A k type main sequence star also referred to as a k dwarf or orange dwarf is a main sequence hydrogen burning star of spectral type k and luminosity class v. The surface temperatures of a type stars range from 7400 k to about 10000 k. Class b stars typically range from 10000 k to 25000 k and are also bluish white but show neutral helium lines.
Using the letters o b a f g k and m stars are easily classified from hottest o to coolest m. Giant and supergiant stars old large stars. These stars are intermediate in size between red m type main sequence stars red dwarfs and yellow g type main sequence stars.
F type stars are yellow white reach 60007400 k. Most stars are currently classified under the morgan keenan mk system using the letters o b a f g k and m a sequence from the hottest o type to the coolest m type. The spectral class of a star is a short code primarily summarizing the ionization state giving an objective measure of the photospheres temperature.
Proxima centauri is a red dwarf. Lines of hydrogen are prominent and these stars are white.
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