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  2. List of proper names of stars - Wikipedia

    en.wikipedia.org/wiki/List_of_proper_names_of_stars

    In 2016, the International Astronomical Union (IAU) organized a Working Group on Star Names (WGSN) [2] to catalog and standardize proper names for stars. The WGSN's first bulletin, dated July 2016, [3] included a table of 125 stars comprising the first two batches of names approved by the WGSN (on 30 June and 20 July 2016) together with names of stars adopted by the IAU Executive Committee ...

  3. Quasi-star - Wikipedia

    en.wikipedia.org/wiki/Quasi-star

    A quasi-star (also called black hole star) is a hypothetical type of extremely large and luminous star that may have existed early in the history of the Universe. They are thought to have existed for around 7–10 million years due to their immense mass .

  4. Dark nebula - Wikipedia

    en.wikipedia.org/wiki/Dark_nebula

    The closest and largest dark nebulae are visible to the naked eye, since they are the least obscured by stars in between Earth and the nebula, and because they have the largest angular size, appearing as dark patches against the brighter background of the Milky Way like the Coalsack Nebula and the Great Rift.

  5. Fixed stars - Wikipedia

    en.wikipedia.org/wiki/Fixed_stars

    The phrase "fixed star" is technically incorrect, but nonetheless it is used in an historical context, and in classical mechanics. When used as a visual reference for observations, they usually are called background stars or simply distant stars, still retaining the intuitive meaning of they being "fixed" in some practical sense.

  6. File:600px White star on Black background.svg - Wikipedia

    en.wikipedia.org/wiki/File:600px_White_star_on...

    File:600px White star on Black background.svg. Add languages. ... Black flag with a white five-pointed star: Date: 12 January 2016, 13:55 UTC+1: Source: Own work: Author:

  7. Portal:Stars - Wikipedia

    en.wikipedia.org/wiki/Portal:Stars

    At the end of a star's lifetime as a fusor, its core becomes a stellar remnant: a white dwarf, a neutron star, or—if it is sufficiently massive—a black hole. Stellar nucleosynthesis in stars or their remnants creates almost all naturally occurring chemical elements heavier than lithium .

  8. Portal:Stars/Black hole - Wikipedia

    en.wikipedia.org/wiki/Portal:Stars/Black_hole

    Star Sun Galaxy Black hole Supernova This page was last edited on 18 June 2021, at 20:06 (UTC). Text is available under ...

  9. Black dwarf - Wikipedia

    en.wikipedia.org/wiki/Black_dwarf

    A black dwarf is a theoretical stellar remnant, specifically a white dwarf that has cooled sufficiently to no longer emit significant heat or light. Because the time required for a white dwarf to reach this state is calculated to be longer than the current age of the universe (13.8 billion years), no black dwarfs are expected to exist in the ...