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  2. Perseus–Pisces Supercluster - Wikipedia

    en.wikipedia.org/wiki/Perseus–Pisces_Supercluster

    The Perseus–Pisces Supercluster is one of two dominant concentrations of galaxies (the other being the Local supercluster) in the nearby universe (within 300 million light years). This supercluster also borders a prominent void, the Taurus Void, and is part of the Perseus–Pegasus Filament which stretches for roughly a billion light years. [1]

  3. Pisces–Cetus Supercluster Complex - Wikipedia

    en.wikipedia.org/wiki/Pisces–Cetus_Supercluster...

    The Pisces–Cetus Supercluster Complex is estimated to be about 1.0 billion light-years (Gly) long and 150 million light years (Mly) wide. It is one of the largest structures known in the observable universe, but is exceeded by the Sloan Great Wall (1.3 Gly), Clowes–Campusano LQG (2.0 Gly), U1.11 LQG (2.5 Gly), Huge-LQG (4.0 Gly), and Hercules–Corona Borealis Great Wall (10 Gly ...

  4. List of largest cosmic structures - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_cosmic...

    This galaxy filament contains the Perseus–Pisces Supercluster. Pisces–Cetus Supercluster Complex (1987) 1,000,000,000: Contains the Milky Way, and is the first galaxy filament to be discovered. (The first LQG was found earlier in 1982.) A new report in 2014 confirms the Milky Way as a member of the Laniakea Supercluster. CfA2 Great Wall ...

  5. Supercluster - Wikipedia

    en.wikipedia.org/wiki/Supercluster

    The most massive galaxy supercluster discovered until 2023. [10] Laniakea Supercluster: z = 0.000; Length = 153 Mpc (500 million light-years) The Laniakea Supercluster is the supercluster that contains the Virgo Cluster, Local Group, and by extension on the latter, our galaxy; the Milky Way. [2] Virgo Supercluster: z= 0.000

  6. Galaxy filament - Wikipedia

    en.wikipedia.org/wiki/Galaxy_filament

    Discovery of structures larger than superclusters began in the late 1980s. In 1987, astronomer R. Brent Tully of the University of Hawaii's Institute of Astronomy identified what he called the Pisces–Cetus Supercluster Complex. The CfA2 Great Wall was discovered in 1989, [6] followed by the Sloan Great Wall in 2003. [7]

  7. Category:Pisces–Cetus Supercluster Complex - Wikipedia

    en.wikipedia.org/wiki/Category:Pisces–Cetus...

    Perseus-Pisces Supercluster (2 C, 7 P) Pages in category "Pisces–Cetus Supercluster Complex" The following 2 pages are in this category, out of 2 total.

  8. Category:Perseus-Pisces Supercluster - Wikipedia

    en.wikipedia.org/wiki/Category:Perseus-Pisces...

    Pages in category "Perseus-Pisces Supercluster" The following 7 pages are in this category, out of 7 total. This list may not reflect recent changes. ...

  9. Laniakea Supercluster - Wikipedia

    en.wikipedia.org/wiki/Laniakea_Supercluster

    Local Supercluster, Laniakea, Laniakea Supercluster, Laniakea Complex The Laniakea Supercluster ( / ˌ l ɑː n i . ə ˈ k eɪ . ə / ; Hawaiian for "open skies" or "immense heaven") [ 2 ] or the Local Supercluster ( LSC or LS ) is the galaxy supercluster that is home to the Milky Way and approximately 100,000 other nearby galaxies.