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  2. Red supergiant - Wikipedia

    en.wikipedia.org/wiki/Red_supergiant

    Red supergiants develop deep convection zones reaching from the surface over halfway to the core and these cause strong enrichment of nitrogen at the surface, with some enrichment of heavier elements. [26] Some red supergiants undergo blue loops where they temporarily increase in temperature before returning to the red supergiant state. This ...

  3. List of nearest supergiants - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_supergiants

    While it is frequently described as a yellow supergiant, especially in evolutionary terms, [2] it is classified as a bright giant based on spectrum. [3] Sargas (θ Scorpii A) 329 ± 9 [5] F0Ib-F1III [6] or F0 II [7] 35.5 × 26.3 [5] 3.1 +0.37 −0.32 [5] 1.862 [8] Either a lower luminosity supergiant or a (bright) giant, formed after stellar ...

  4. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    In these lists are some examples of extremely distant extragalactic stars, which may have slightly different properties and natures than the currently largest known stars in the Milky Way. For example, some red supergiants in the Magellanic Clouds are suspected to have slightly different limiting temperatures and luminosities.

  5. Supergiant - Wikipedia

    en.wikipedia.org/wiki/Supergiant

    Post-red supergiant stars have a generally higher level of nitrogen relative to carbon due to convection of CNO-processed material to the surface and the complete loss of the outer layers. Surface enhancement of helium is also stronger in post-red supergiants, representing more than a third of the atmosphere. [28] [29]

  6. Giant star - Wikipedia

    en.wikipedia.org/wiki/Giant_star

    Red giants include stars in a number of distinct evolutionary phases of their lives: a main red-giant branch (RGB); a red horizontal branch or red clump; the asymptotic giant branch (AGB), although AGB stars are often large enough and luminous enough to get classified as supergiants; and sometimes other large cool stars such as immediate post ...

  7. Red giant - Wikipedia

    en.wikipedia.org/wiki/Red_giant

    Another noteworthy feature of red giants is that, unlike Sun-like stars whose photospheres have a large number of small convection cells (solar granules), red-giant photospheres, as well as those of red supergiants, have just a few large cells, the features of which cause the variations of brightness so common on both types of stars. [8]

  8. Category:Red giants - Wikipedia

    en.wikipedia.org/wiki/Category:Red_giants

    A red giant is a luminous giant star of low or intermediate mass that is in a late phase of its evolution. Subcategories. This category has the following 7 ...

  9. Category:Supergiants - Wikipedia

    en.wikipedia.org/wiki/Category:Supergiants

    Supergiants are stars of luminosity class I. Luminosity class Ib is for normal supergiants; Luminosity class Ia is for bright supergiants; Luminosity class Iab is for ...