Astronomy and Space

Horizontal branch

The horizontal branch (HB) is a stage of stellar evolution that immediately follows the red-giant branch in stars whose masses are similar to the Sun's. Horizontal-branch stars are powered by helium fusion in the core (via the triple-alpha process) and by hydrogen fusion (via the CNO cycle) in a shell surrounding the core. The onset of core helium fusion at the tip of the red-giant branch causes substantial changes in stellar structure, resulting in an overall reduction in luminosity, some contraction of the stellar envelope, and the surface reaching higher temperatures.

Also on this shelf

See also

• ▸Eta Ceti
• ▸2nd Armoured Division (United Kingdom)
• ▸Climate of Titan

Uncatalogued shelf

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