Giant star
A giant star is a star with much larger radius and luminosity than a main-sequence star of the same surface temperature.[2][3]
Giant stars are up to a few hundred times the diameter of the Sun and between 10 and a few thousand times brighter than the Sun. They don't last as long as most main sequence stars. Stars still more luminous than giants are referred to as supergiants and hypergiants.
A hot, luminous main-sequence star may also be referred to as a giant.[4]
There are a wide range of giant class stars, and sub-divisions are often used to identify particular types. Astronomers use such terms as: sub-giants, bright giants, red giants, yellow giants and blue giants. The giant luminosity class is given the Roman numeral III, for bright giants it is II.
Types of giants
[change | change source]Red giants
[change | change source]These have spectral types K to M.
Yellow giants
[change | change source]These have spectral types F and G.
- Capella A and B
The Cepheid variables are yellow giants.
Blue giants
[change | change source]These have spectral types A, B, and O.
Bright giants
[change | change source]Giants nearly as bright as supergiants. They can have many spectral types.
References
[change | change source]- ↑ Richard Powell with permission.
- ↑ Giant star. In Astronomy Encyclopedia, ed. Patrick Moore, New York: Oxford University Press, 2002. ISBN 0-19-521833-7
- ↑ Giant. In The Facts on File Dictionary of Astronomy, ed. John Daintith and William Gould. 5th ed, New York: Facts On File, 2006. ISBN 0-8160-5998-5
- ↑ Giant star. In Cambridge Dictionary of Astronomy, Mitton, Jacqueline. Cambridge University Press 2001. ISBN 0-521-80045-5