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  2. 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.

  3. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    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 Cloud L/T eff: An unusual blue hypergiant with a large dusty disk. [128] R136a1: 42.7 +1.6 −0.9 [129] Large Magellanic Cloud L/T eff

  4. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    Betelgeuse is a red supergiant star in the constellation of Orion. It is usually the tenth-brightest star in the night sky and, after Rigel, the second-brightest in its constellation. It is a distinctly reddish, semiregular variable star whose apparent magnitude, varying between +0.0 and +1.6, has the widest range displayed by any first ...

  5. Amandaland star Lucy Punch: ‘My list of failures? I did a ...

    www.aol.com/amandaland-star-lucy-punch-list...

    INTERVIEW: After decades of playing posh, smug supporting roles, comic actor Punch finally has the opportunity to star as a posh, smug lead in her own BBC show, ‘Amandaland’. She tells Hannah ...

  6. List of most massive stars - Wikipedia

    en.wikipedia.org/wiki/List_of_most_massive_stars

    It is the most massive star that has a Bayer designation. It was only discovered to be (at least) two stars in the past few decades. Both the obscuring clouds and the great distances also make it difficult to judge whether the star is just a single supermassive object or, instead, a multiple star system. A number of the "stars" listed below may ...

  7. NGC 1746 - Wikipedia

    en.wikipedia.org/wiki/NGC_1746

    NGC 1746 is a sparse, large star grouping that spans around 40 arcminutes. Originally classified as an open cluster, later studies suggest it is likely to be an asterism. NGC 1750 is a true open star cluster, spanning 20 arcminutes, with an estimated age of 150–200 million years. It contains several dozen stars, many of which are still on the ...