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  2. Template:Scorpius - Wikipedia

    en.wikipedia.org/wiki/Template:Scorpius

    } is a {}-based template to be used at the bottom of articles about astronomical objects beyond the Solar System, located in the constellation of Scorpius. The template is divided into categories of stars , star clusters , nebulae , exoplanets , galaxies , galaxy clusters , and a miscellaneous "other" category.

  3. Scorpius - Wikipedia

    en.wikipedia.org/wiki/Scorpius

    The close pair of stars ω 1 Scorpii and ω² Scorpii are an optical double, which can be resolved by the unaided eye. One is a yellow giant, [9] while the other is a blue B-type star in the Scorpius-Centaurus Association. [10] The star once designated γ Sco (despite being well within the boundaries of Libra) is today known as σ Lib.

  4. List of stars in Scorpius - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_in_Scorpius

    • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] See also [ edit ]

  5. Category:Scorpius - Wikipedia

    en.wikipedia.org/wiki/Category:Scorpius

    Printable version; In other projects ... Pages in category "Scorpius" ... This list may not reflect recent changes. Scorpius * List of stars in Scorpius; 0–9. 1 ...

  6. Zeta1 Scorpii - Wikipedia

    en.wikipedia.org/wiki/Zeta1_Scorpii

    Zeta 1 Scorpii (Zeta 1 Sco, ζ 1 Scorpii, ζ 1 Sco) is a B-type hypergiant star in the constellation of Scorpius. [9] It has an apparent visual magnitude which varies between 4.66 and 4.86. [ 3 ] It is a member of the Scorpius OB1 association , and potentially of the open star cluster NGC 6231 , [ 11 ] also known as the "Northern jewel box ...

  7. Nu Scorpii - Wikipedia

    en.wikipedia.org/wiki/Nu_Scorpii

    Nu Scorpii (ν Scorpii, abbreviated Nu Sco, ν Sco) is a multiple star system in the constellation of Scorpius. It is most likely a septuple star system, [5] consisting of two close groups (designated Nu Scorpii AB and CD) that are separated by 41 arcseconds. [5] Based on parallax measurements, [7] it is approximately 470 light-years from the Sun.