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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. Category:Perseus-Pisces Supercluster - Wikipedia

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

    Perseus–Pisces Supercluster; 0–9. 3C 66B; A. Abell 262; N. NGC 498; NGC 7003; NGC 7836; P. Perseus Cluster This page was last edited on 18 October 2022, at 19:42 ...

  4. Perseus Cluster - Wikipedia

    en.wikipedia.org/wiki/Perseus_Cluster

    The Perseus cluster (Abell 426) is a cluster of galaxies in the constellation Perseus. It has a recession speed of 5,366 km/ s and a diameter of 863 ′ . [ 1 ] It is one of the most massive objects in the known universe , containing thousands of galaxies immersed in a vast cloud of multimillion-degree gas.

  5. Category:Perseus Cluster - Wikipedia

    en.wikipedia.org/wiki/Category:Perseus_Cluster

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  6. Perseus–Pegasus Filament - Wikipedia

    en.wikipedia.org/wiki/Perseus–Pegasus_Filament

    The Perseus–Pegasus Filament is a galaxy filament containing the Perseus–Pisces Supercluster and stretching for roughly a billion light-years (or over 300/h Mpc). Currently, it is considered to be one of the largest known structures in the universe. [note 1] This filament is adjacent to the Pisces–Cetus Supercluster Complex. [1] [2]

  7. 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 ...

  8. Binocular disparity - Wikipedia

    en.wikipedia.org/wiki/Binocular_disparity

    The disparity of the images on the actual retina depends on factors internal to the eye, especially the location of the nodal points, even if the cross section of the retina is a perfect circle. Disparity on retina conforms to binocular disparity when measured as degrees, while much different if measured as distance due to the complicated ...

  9. NGC 1275 - Wikipedia

    en.wikipedia.org/wiki/NGC_1275

    NGC 1275 (also known as Perseus A or Caldwell 24) is a type 1.5 Seyfert galaxy [3] located around 237 million light-years away [2] in the direction of the constellation Perseus. NGC 1275 is a member of the large Perseus Cluster of galaxies.