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  2. 6 Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/6_Cassiopeiae

    6 Cassiopeiae A is a white A2.5 type hypergiant. It is about 25 times as massive as the Sun and 200,000 times as luminous. The star is slightly and erratically variable, an Alpha Cygni variable.

  3. Hypergiant - Wikipedia

    en.wikipedia.org/wiki/Hypergiant

    A hypergiant (luminosity class 0 or Ia +) is a very rare type of star that has an extremely high luminosity, mass, size and mass loss because of its extreme stellar winds. The term hypergiant is defined as luminosity class 0 (zero) in the MKK system .

  4. Hypergiant Industries - Wikipedia

    en.wikipedia.org/wiki/Hypergiant_Industries

    Hypergiant is an Austin, Texas based technology company, [5] founded in February 2018, [4] and currently headed by CEO Mike Betzer. [ 3 ] [ 6 ] The company develops artificial intelligence (AI) products, [ 7 ] focused on its CommandCenter Platform.

  5. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    A yellow hypergiant. HD 271182: 621 [126] Large Magellanic Cloud L/T eff: A yellow hypergiant. HD 33579: 471 [124] Large Magellanic Cloud L/T eff: The brightest star in the Large Magellanic Cloud. S Doradus: 100 [127] Large Magellanic Cloud L/T eff: A luminous blue variable in the S Doradus instability strip. HD 37974: 99 [128] Large Magellanic ...

  6. Rho Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/Rho_Cassiopeiae

    Rho Cassiopeiae (/ ˌ r oʊ k æ s i ə ˈ p iː aɪ,-s i oʊ-,-iː /; ρ Cas, ρ Cassiopeiae) is a yellow hypergiant star in the constellation Cassiopeia.It is about 8,150 light-years (2,500 pc) from Earth, yet can still be seen by the naked eye as it is over 300,000 times brighter than the Sun.

  7. Stephenson 2 DFK 1 - Wikipedia

    en.wikipedia.org/wiki/Stephenson_2_DFK_1

    Stephenson 2 DFK 1, also known as RSGC2-01 [a] or St2-18, is a red supergiant (RSG) or possible extreme red hypergiant [2] (RHG) star in the constellation of Scutum.It lies near the open cluster Stephenson 2, which is located about 5.8 kiloparsecs (19,000 light-years) away from Earth in the Scutum–Centaurus Arm of the Milky Way galaxy, and is assumed to be one of a group of stars at a ...

  8. Giant star - Wikipedia

    en.wikipedia.org/wiki/Giant_star

    A giant star has a substantially larger radius and luminosity than a main-sequence (or dwarf) star of the same surface temperature. [1] They lie above the main sequence (luminosity class V in the Yerkes spectral classification) on the Hertzsprung–Russell diagram and correspond to luminosity classes II and III. [2]

  9. Luminous blue variable - Wikipedia

    en.wikipedia.org/wiki/Luminous_blue_variable

    Wray 17-96 (unusual hypergiant in the gap between the two semi-stable LBV regions) Pistol Star (once thought to be the most luminous star in the galaxy) LBV 1806-20 (one of the most luminous stars known) Sanduleak -69° 202 (the star that exploded as SN 1987A) Cygnus OB2-12 (blue hypergiant and one of the most luminous stars known) HD 80077 ...

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