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  2. Boötes Void - Wikipedia

    en.wikipedia.org/wiki/Boötes_Void

    A map of the Boötes Void. The Boötes Void (/ b oʊ ˈ oʊ t iː z / boh-OH-teez) (colloquially referred to as the Great Nothing) [1] is an approximately spherical region of space found in the vicinity of the constellation Boötes, containing only 60 galaxies instead of the 2,000 that should be expected from an area this large, hence its name.

  3. List of voids - Wikipedia

    en.wikipedia.org/wiki/List_of_voids

    Name Coordinates Distance Diameter Data Notes Local Void: 18 h 38 m +18° : cz=2500 km/s : 60 Mpc [1]Northern Local Supervoid: 61 Mpc 104 Mpc Virgo Supercluster, Coma Supercluster, Perseus–Pisces Supercluster, Ursa Major–Lynx Supercluster, Hydra–Centaurus Supercluster, Sculptor Supercluster, Pavo–Corona Australes Supercluster form a sheet between the Northern Local Supervoid and the ...

  4. Epsilon Boötis - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Boötis

    Epsilon Boötis (ε Boötis, abbreviated Epsilon Boo, ε Boo), officially named Izar (/ ˈ aɪ z ɑːr / EYE-zar), [16] is a binary star in the northern constellation of Boötes.The star system can be viewed with the unaided eye at night, but resolving the pair with a small telescope is challenging; an aperture of 76 mm (3.0 in) or greater is required.

  5. Boötes - Wikipedia

    en.wikipedia.org/wiki/Boötes

    The star is of type K0 and is located 110 parsecs from Earth; it appears at a visual magnitude of 7.96. It is significantly larger than the Sun, with a mass of 1.61 M ☉ and a radius of 4.6 solar radii. Its one planet, discovered in 2011 by the radial velocity method, has a mass of 2.2 M J; its radius is as yet undetermined. HD 131496 b orbits ...

  6. Tau Boötis - Wikipedia

    en.wikipedia.org/wiki/Tau_Boötis

    Tau Boötis B (with a capital B, as opposed to the planet) is a dim, 11 mag red dwarf with only about half the mass and radius of the Sun. It orbits the primary star at an average distance of about 220 AU (14 arcseconds ) but comes as close as about 28 AU to the primary, giving its orbit a very high eccentricity of about 0.87.

  7. Eta Boötis - Wikipedia

    en.wikipedia.org/wiki/Eta_Boötis

    η Boötis (Latinised to Eta Boötis) is the binary pair's Bayer designation; η Boötis A and B those of its two components. The designations of the two constituents of the double pair as WDS J13547+1824A and B and those of A's components - Aa and Ab - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International ...

  8. Interstitial site - Wikipedia

    en.wikipedia.org/wiki/Interstitial_site

    An octahedral void could fit an atom with a radius 0.414 times the size of the atoms making up the lattice. [1] An atom that fills this empty space could be larger than this ideal radius ratio, which would lead to a distorted lattice due to pushing out the surrounding atoms, but it cannot be smaller than this ratio.

  9. Great void - Wikipedia

    en.wikipedia.org/wiki/Great_void

    At the Edge of the Great Void, the nineteenth volume of the Valérian and Laureline series; A region in the Crystalicum RPG card game "Eoarchaean: The Great Void", a song by The Ocean Collective, from the album Precambrian; Greetings from the Great Void, an album from the Italian duo My Cat Is an Alien; Purgatory in the after-life