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  2. File:A large blank world map with oceans marked in blue.svg

    en.wikipedia.org/wiki/File:A_large_blank_world...

    Blank political world map with blue oceans, fit to replace File:A large blank world map with oceans marked in blue.PNG. Date: 25 July 2006: Source: World Map Blank.svg: Author: Petr Dlouhý: Other versions: Derivative works of this file: Carte Coffea robusta arabic.svg; Hantaviren weltweit.svg; OttomanEmpireIn1683.png

  3. List of largest galaxies - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_galaxies

    Listed below are galaxies with diameters greater than 700,000 light-years. This list uses the mean cosmological parameters of the Lambda-CDM model based on results from the 2015 Planck collaboration, where H 0 = 67.74 km/s/Mpc, Ω Λ = 0.6911, and Ω m = 0.3089. [3]

  4. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    HD 33579: 471 [125] Large Magellanic Cloud L/T eff: The brightest star in the Large Magellanic Cloud. S Doradus: 100 [128] Large Magellanic Cloud L/T eff: A luminous blue variable in the S Doradus instability strip. HD 37974: 99 [129] Large Magellanic Cloud L/T eff: An unusual blue hypergiant with a large dusty disk. [129] R136a1: 42.7 +1.6 − ...

  5. CMB cold spot - Wikipedia

    en.wikipedia.org/wiki/CMB_cold_spot

    The mean ISW imprint 50 supervoids have on the Cosmic Microwave Background: [9] [clarification needed] color scale from -20 to +20 μK.. One possible explanation of the cold spot is a huge void between us and the primordial CMB.

  6. Cetus - Wikipedia

    en.wikipedia.org/wiki/Cetus

    Cetus is not among the 12 true zodiac constellations in the J2000 epoch, nor classical 12-part zodiac.The ecliptic passes less than 0.25° from one of its corners. Thus the Moon and planets will enter Cetus (occulting any stars as a foreground object) in 50% of their successive orbits briefly and the southern part of the Sun appears in Cetus for about one day each year.

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  8. BOSS Great Wall - Wikipedia

    en.wikipedia.org/wiki/BOSS_Great_Wall

    The elongated superclusters form galaxy walls, with the larger of the two having a diameter of 186/h Mpc (supercluster A in the figure); the second wall's being 173/h Mpc (supercluster B). The other two main superclusters are moderately large, having diameters of 91/h Mpc and 64/h Mpc (superclusters D and C, respectively).

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