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  2. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    Theoretical limit of star size (Large Magellanic Cloud) ≳1,550 [11] L/T eff: Estimated by measuring the fraction of red supergiants at higher luminosities in a large sample of stars. Assumes an effective temperature of 3,545 K. Reported for reference: HV 888 1,477 [107] –1,584 [108] Large Magellanic Cloud L/T eff: HD 269551 A 1,439 [109 ...

  3. List of most massive stars - Wikipedia

    en.wikipedia.org/wiki/List_of_most_massive_stars

    Some stars may once have been more massive than they are today. It is likely that many large stars have suffered significant mass loss (perhaps as much as several tens of solar masses). This mass may have been expelled by superwinds: high velocity winds that are driven by the hot photosphere into interstellar space. The process forms an ...

  4. UY Scuti - Wikipedia

    en.wikipedia.org/wiki/UY_Scuti

    UY Scuti (BD-12°5055) is a red supergiant star, located 5,900 light-years away in the constellation Scutum.It is also a pulsating variable star, with a maximum brightness of magnitude 8.29 and a minimum of magnitude 10.56, which is too dim for naked-eye visibility.

  5. List of nearest giant stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_giant_stars

    Print/export Download as PDF; Printable version; In other projects Wikidata item; ... The nearest M-type red giant, and the 25th brightest star in the night sky.

  6. Lists of stars - Wikipedia

    en.wikipedia.org/wiki/Lists_of_stars

    Print/export Download as PDF ... EBLM J0555-57Ab — is one of the smallest stars ever discovered. ... and large-scale structure; Timeline of white dwarfs, neutron ...

  7. 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]

  8. Supergiant - Wikipedia

    en.wikipedia.org/wiki/Supergiant

    Rigel, the brightest star in the constellation Orion is a typical blue-white supergiant; the three stars of Orion's Belt are all blue supergiants; Deneb is the brightest star in Cygnus, another blue supergiant; and Delta Cephei (itself the prototype) and Polaris are Cepheid variables and yellow supergiants.

  9. S Doradus - Wikipedia

    en.wikipedia.org/wiki/S_Doradus

    S Doradus (also known as S Dor) is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, located roughly 160,000 light-years away. The star is a luminous blue variable , and one of the most luminous stars known , having a luminosity varying widely above and below 1,000,000 times the luminosity of ...