Red giant

According to the Hertzsprung-Russell diagram, a red giant is a large non-main sequence star of stellar classification K or M; so-named because of the reddish appearance of the cooler "giants". Examples include Aldebaran and Arcturus.

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They are believed to be stars of solar mass or higher which have exhausted the supply of hydrogen in their cores and started fusing hydrogen in a shell outside the core. Since the source of

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energy is closer to the surface, the star begins to expand. This makes

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the star more luminous (from 1,000 - 10,000 times brighter) but, counterintuitively, also reduces the effective temperature. This is because the radius (and hence surface area) of the star increases by a larger amount than the luminosity of the star. As a result, the star becomes larger, but cooler and redder—hence red giant.

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If the star is less than 2.5 solar masses, the addition of helium to the core by shell hydrogen fusing will cause a helium flash—a rapid burst

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of helium fusing in the core, after which the star will commence a brief period of helium fusing before beginning another ascent of the red giant branch. Stars more massive than 2.5 solar masses enter the helium fusing phase of their lives much more smoothly. The core helium fusing phase of a star's life is called the horizontal branch in metal-poor stars, so named because these stars lie on a nearly horizontal line in the Hertzsprung-Russell diagram of many star clusters. Metal-rich helium-fusing stars do not lie on a horizontal branch, but instead lie in a clump (the red clump) in the Hertzsprung-Russell diagram.

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Stars may enter a red giant phase several times if they are capable of fusing elements more massive than helium in their cores. In these cases, the star is then on the asymptotic giant branch.

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Hertzsprung-Russell diagram: In stellar astronomy, the Hertzsprung-Russell diagram (usually referred to by the abbreviation H-R diagram or HRD) shows the relationship between absolute magnitude, luminosity, stellar classification, and surface temperature. This was devised, c.1910, by Ejnar Hertzsprung and Henry Norris Russell....

Main sequence: The main sequence of the Hertzsprung-Russell diagram is the curve where the majority of stars are located in this diagram. Stars located on this band are known as main-sequence stars or dwarf stars. The coolest dwarfs are the red dwarfs....

Star: :This article is about celestial bodies....

Red giant related Images and Photos (experimental)

The Giant Red Doors to the Forbidden City in Beijing	Boston Red Sox Giant Floor Puzzle	Giant	Red
Red	Red	Imagine (Red)	Red I
Red M&M	Red II	Red II	Red III