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  2. MilkyWay@home - Wikipedia

    en.wikipedia.org/wiki/MilkyWay@home

    MilkyWay@home is a volunteer computing project in the astrophysics category, running on the Berkeley Open Infrastructure for Network Computing (BOINC) platform. Using spare computing power from over 38,000 computers run by over 27,000 active volunteers as of November 2011, the MilkyWay@home project aims to generate accurate three-dimensional dynamic models of stellar streams in the immediate ...

  3. The Berkeley Open Infrastructure for Network Computing [2] ( BOINC, pronounced / bɔɪŋk / – rhymes with "oink" [3]) is an open-source middleware system for volunteer computing (a type of distributed computing ). [4] Developed originally to support SETI@home, [5] it became the platform for many other applications in areas as diverse as ...

  4. Category:Milky Way Subgroup - Wikipedia

    en.wikipedia.org/wiki/Category:Milky_Way_Subgroup

    Pages in category "Milky Way Subgroup" The following 44 pages are in this category, out of 44 total. This list may not reflect recent changes. *

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  6. Carina–Sagittarius Arm - Wikipedia

    en.wikipedia.org/wiki/Carina–Sagittarius_Arm

    Observed structure of the Milky Way 's spiral arms. The Carina–Sagittarius Arm (also known as the Sagittarius Arm or Sagittarius–Carina Arm, labeled -I [clarification needed]) is generally thought to be a minor spiral arm of the Milky Way galaxy. [1] Each spiral arm is a long, diffuse curving streamer of stars that radiates from the ...

  7. The Cowherd and the Weaver Girl - Wikipedia

    en.wikipedia.org/wiki/The_Cowherd_and_the_Weaver...

    The heavenly river ( Milky Way) separates them. The Cowherd and the Weaver Girl are characters found in Chinese mythology and appear eponymously in a romantic Chinese folk tale. The story tells of the romance between Zhinü ( 織女; the weaver girl, symbolized by the star Vega) and Niulang ( 牛郎; the cowherd, symbolized by the star Altair ...

  8. Magellanic Clouds - Wikipedia

    en.wikipedia.org/wiki/Magellanic_Clouds

    The Magellanic Clouds ( Magellanic system [2] [3] or Nubeculae Magellani [4]) are two irregular dwarf galaxies in the southern celestial hemisphere. Orbiting the Milky Way galaxy, these satellite galaxies are members of the Local Group. Because both show signs of a bar structure, they are often reclassified as Magellanic spiral galaxies.

  9. Satellite galaxies of the Milky Way - Wikipedia

    en.wikipedia.org/wiki/Satellite_galaxies_of_the...

    The Milky Way has several smaller galaxies gravitationally bound to it, as part of the Milky Way subgroup, which is part of the local galaxy cluster, the Local Group.. There are 61 small galaxies confirmed to be within 420 kiloparsecs (1.4 million light-years) of the Milky Way, but not all of them are necessarily in orbit, and some may themselves be in orbit of other satellite galaxies.