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  2. Shape of the universe - Wikipedia

    en.wikipedia.org/wiki/Shape_of_the_universe

    Global geometry: This pertains to the universe's overall shape and structure. The observable universe (of a given current observer) is a roughly spherical region extending about 46 billion light-years in all directions (from that observer, the observer being the current Earth, unless specified otherwise). [3]

  3. List of largest cosmic structures - Wikipedia

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

    Discovered through gamma-ray burst mapping. Largest-known regular formation in the observable universe. [8] Huge-LQG (2012–2013) 4,000,000,000 [9] [10] [11] Decoupling of 73 quasars. Largest-known large quasar group and the first structure found to exceed 3 billion light-years. "The Giant Arc" (2021) 3,300,000,000 [12] Located 9.2 billion ...

  4. Pablo Vegetti - Wikipedia

    en.wikipedia.org/wiki/Pablo_Vegetti

    Pablo Vegetti; Personal information; Full name: Pablo Ezequiel Vegetti Pfaffen: Date of birth 15 October 1988 (age 36) Place of birth: Santa Fe, Argentina: Height: 1.88 m (6 ft 2 in) Position(s) Forward: Team information

  5. Observable universe - Wikipedia

    en.wikipedia.org/wiki/Observable_universe

    The universe's size is unknown, and it may be infinite in extent. [14] Some parts of the universe are too far away for the light emitted since the Big Bang to have had enough time to reach Earth or space-based instruments, and therefore lie outside the observable universe. In the future, light from distant galaxies will have had more time to ...

  6. Void (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Void_(astronomy)

    This means that the evolution of a void's shape is in part the result of the expansion of the universe. Since this acceleration is believed to be caused by dark energy, studying the changes of a void's shape over a period of time can be used to constrain the standard Λ CDM model, [ 36 ] [ 37 ] or further refine the Quintessence + Cold Dark ...

  7. Flatness problem - Wikipedia

    en.wikipedia.org/wiki/Flatness_problem

    The local geometry of the universe is determined by whether the relative density Ω is less than, equal to or greater than 1. From top to bottom: a spherical universe with greater than critical density (Ω>1, k>0); a hyperbolic, underdense universe (Ω<1, k<0); and a flat universe with exactly the critical density (Ω=1, k=0).

  8. Michael Weatherly and Cote de Pablo Set to Reprise 'NCIS ...

    www.aol.com/entertainment/michael-weatherly-cote...

    Weatherly, 55, and de Pablo, 44, will reprise their respective fan-favorite roles, Tony DiNozzo and Ziva David, in an unnamed spinoff series ordered by Paramount +, the streaming platform revealed ...

  9. Large quasar group - Wikipedia

    en.wikipedia.org/wiki/Large_quasar_group

    A large quasar group (LQG) is a collection of quasars (a form of supermassive black hole active galactic nuclei) that form what are thought to constitute the largest astronomical structures in the observable universe. LQGs are thought to be precursors to the sheets, walls and filaments of galaxies found in the relatively nearby universe. [1]