Astrophysics (index)about

giant star

(star larger than main sequence stars)

A giant star is a star much larger than a main sequence star, whose radius is on the order of an astronomical unit. After the main sequence, stars go through phases where they become giants, e.g., red giant or a star on the asymptotic giant branch.

The name originally applied to especially bright stars, i.e., a large luminosity or absolute magnitude. Because the brightness is directly related to the area facing us (the square of the radius), the brightest stars are indeed large, known as bright giants or for even brighter, supergiants. The general term dwarf star actually applies to any star that is not a giant (e.g., the Sun), though sometimes "dwarf" is used with a qualifier to signify a more specific meaning (white dwarf, red dwarf, brown dwarf).

(star type,stellar evolution)

Referenced by:
asymptotic giant branch (AGB)
black hole merger
binary star
bolometric correction
H-R diagram (HRD)
instability strip
isothermal core
L-type star (L)
luminosity class
main sequence star
post main sequence star
Palomar Testbed Interferometer (PTI)
red giant
red-giant branch (RGB)
stellar age determination
stellar core
S-type star
surface gravity
symbiotic binary
Thorne-Żytkow object (TZO)