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  2. Super Giant - Wikipedia

    en.wikipedia.org/wiki/Super_Giant

    Super Giant (スーパージャイアンツ, Sūpā Jaiantsu, literally translated as "Super Giants") is a Japanese superhero featured in a successful series of serial-like tokusatsu short feature films produced between 1957 and 1959 by Shintoho (the non-union branch of Toho).

  3. List of nearest supergiants - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_supergiants

    Some of the brightest stars in the night sky, such as Rigel and Antares, are in the list. While supergiants are typically defined as stars with luminosity classes Ia, Iab or Ib, other definitions exist, such as those based on stellar evolution. [1] Therefore, stars with other luminosity classes can sometimes be considered supergiants.

  4. Supergiant - Wikipedia

    en.wikipedia.org/wiki/Supergiant

    One region contained larger and more luminous stars of spectral types A to M and received the name giant. [1] Subsequently, as they lacked any measurable parallax, it became apparent that some of these stars were significantly larger and more luminous than the bulk, and the term super-giant arose, quickly adopted as supergiant. [2] [3] [4]

  5. Category:Supergiants - Wikipedia

    en.wikipedia.org/wiki/Category:Supergiants

    Afrikaans; Беларуская (тарашкевіца) Bosanski; Català; Čeština; Ελληνικά; Español; Esperanto; Euskara; فارسی; Français; Galego

  6. List of nearest giant stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_giant_stars

    The nearest white giant. Capella A 42.919 ± 0.049 [9] G8III [9] 11.98 ± 0.57 [9] 2.5687 [9] 0.03 [10] The nearest yellow giant, together with Capella A. With a magnitude of 0.08, [11] the Capella star system is the 6th-brightest star in the night sky. Capella B G0III [9] 8.83 ± 0.33 [9] 2.48 [9] 0.16 [10] The nearest yellow giant, together ...

  7. Super-AGB star - Wikipedia

    en.wikipedia.org/wiki/Super-AGB_star

    Colour-Magnitude Diagram showing evolutionary tracks for stars in the super-AGB mass range. A super-AGB star is a star with a mass intermediate between those that end their lives as a white dwarf and those that end with a core collapse supernova, and properties intermediate between asymptotic giant branch (AGB) stars and red supergiants.

  8. Category:G-type supergiants - Wikipedia

    en.wikipedia.org/wiki/Category:G-type_supergiants

    G-type supergiants are supergiant (luminosity class I) stars of spectral type G. Pages in category "G-type supergiants" The following 58 pages are in this category, out of 58 total.

  9. List of star extremes - Wikipedia

    en.wikipedia.org/wiki/List_of_star_extremes

    All stars closer to the Sun are main sequence or degenerate stars or brown dwarfs. Nearest undisputed subgiant Delta Pavonis: 19.9 light-years (6.1 pc) A subgiant, but only slightly brighter than the Sun. Nearest "true" giant star Pollux: 33.8 light-years (10.4 pc) List of nearest giant stars: Nearest red giant: Arcturus: 36.7 light-years (11.3 pc)