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  2. 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.

  3. Yellow hypergiant - Wikipedia

    en.wikipedia.org/wiki/Yellow_hypergiant

    Intrinsic variable types in the Hertzsprung–Russell diagram showing the Yellow Hypergiants above (i.e. more luminous than) the Cepheid instability strip. A yellow hypergiant (YHG) is a massive star with an extended atmosphere, a spectral class from A to K, and, starting with an initial mass of about 20–60 solar masses, has lost as much as half that mass.

  4. Red supergiant - Wikipedia

    en.wikipedia.org/wiki/Red_supergiant

    Some red supergiants are larger and more luminous, with radii exceeding over a thousand times that of the Sun. These are hence also referred to as red hypergiants: Mu Cephei; VV Cephei A; NML Cygni; S Persei; UY Scuti; VY Canis Majoris; Westerlund 1 W26; WOH G64: transitioned into a yellow hypergiant in 2014. [33] KY Cygni; BI Cygni

  5. HR 5171 - Wikipedia

    en.wikipedia.org/wiki/HR_5171

    HR 5171, also known as V766 Centauri, is a yellow hypergiant in the constellation Centaurus. It is said to be either an extreme red supergiant (RSG) or recent post-red supergiant (Post-RSG) yellow hypergiant (YHG), both of which suggest it is one of the largest known stars. The star's diameter is uncertain but likely to be between 1,100 and ...

  6. Red giant - Wikipedia

    en.wikipedia.org/wiki/Red_giant

    Red giants vary in the way by which they generate energy: most common red giants are stars on the red-giant branch (RGB) that are still fusing hydrogen into helium in a shell surrounding an inert helium core; red-clump stars in the cool half of the horizontal branch, fusing helium into carbon in their cores via the triple-alpha process

  7. Late life depression - Wikipedia

    en.wikipedia.org/wiki/Late_life_depression

    Late-life depression is often underdiagnosed, which is due to numerous reasons, including that depressed mood is commonly not as prominent as other somatic and psychotic symptoms such as loss of appetite, disruptions in sleep, lack of energy or anergia, fatigue, and loss of interest and enjoyment in normal life activities.

  8. List of star extremes - Wikipedia

    en.wikipedia.org/wiki/List_of_star_extremes

    Nearest red giant: Arcturus: 36.7 light-years (11.3 pc) Nearest supergiant: Canopus: 309 light-years (95 pc) While it is frequently described as a yellow supergiant, especially in evolutionary terms, [16] it is classified as a bright giant based on spectrum. [17] [16] List of nearest supergiants: Nearest hypergiant: μ Cephei (Herschel's Garnet ...

  9. Mu Cephei - Wikipedia

    en.wikipedia.org/wiki/Mu_Cephei

    Mu Cephei (Latinized from μ Cephei, abbreviated Mu Cep or μ Cep), also known as Herschel's Garnet Star, Erakis, or HD 206936, is a red supergiant or hypergiant [4] [7] star in the constellation Cepheus. It appears garnet red and is located at the edge of the IC 1396 nebula.

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