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  2. File:Milky way profile.svg - Wikipedia

    en.wikipedia.org/wiki/File:Milky_way_profile.svg

    File:Milky way profile.svg. Size of this PNG preview of this SVG file: 573 × 600 pixels. Other resolutions: 229 × 240 pixels | 458 × 480 pixels | 734 × 768 pixels | 978 × 1,024 pixels | 1,956 × 2,048 pixels | 1,681 × 1,760 pixels. This is a file from the Wikimedia Commons. Information from its description page there is shown below.

  3. 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 ...

  4. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    A schematic profile of the Milky Way. Abbreviations: GNP/GSP: Galactic North and South Poles. The Milky Way is approximately 890 billion to 1.54 trillion times the mass of the Sun in total (8.9 × 10 11 to 1.54 × 10 12 solar masses), although stars and planets make up only a small part of this. Estimates of the mass of the Milky Way vary ...

  5. Galactic Center - Wikipedia

    en.wikipedia.org/wiki/Galactic_Center

    Galactic Center. 17 45 40.04, −29° 00′ 28.1″. The Galactic Center, as seen by one of the 2MASS infrared telescopes, is located in the bright upper left portion of the image. Marked location of the Galactic Center. The Galactic Center is the barycenter of the Milky Way and a corresponding point on the rotational axis of the galaxy.

  6. Radcliffe wave - Wikipedia

    en.wikipedia.org/wiki/Radcliffe_wave

    Radcliffe wave. The approximate outline of the Radcliffe wave in Earth's night sky. The Radcliffe wave is a neighbouring coherent gaseous structure in the Milky Way, dotted with a related high concentration of interconnected stellar nurseries. It stretches about 8,800 light years. [1] [2] This structure runs with the trajectory of the Milky Way ...

  7. Galactic disc - Wikipedia

    en.wikipedia.org/wiki/Galactic_disc

    The Sculptor Galaxy (NGC 253) is an example of a disc galaxy. A galactic disc (or galactic disk) is a component of disc galaxies, such as spiral galaxies, lenticular galaxies, and the Milky Way. Galactic discs consist of a stellar component (composed of most of the galaxy's stars) and a gaseous component (mostly composed of cool gas and dust).

  8. Galactic quadrant - Wikipedia

    en.wikipedia.org/wiki/Galactic_quadrant

    Galactic quadrant. Longitudinal lines of the galactic coordinate system. A galactic quadrant, or quadrant of the Galaxy, is one of four circular sectors in the division of the Milky Way Galaxy. Numbered quadrants and sectors of constellations. Quadrants as starcharts, with most prominent stars marked.

  9. Sagittarius Stream - Wikipedia

    en.wikipedia.org/wiki/Sagittarius_Stream

    Sagittarius Stream. In astronomy, the Sagittarius Stream is a long, complex structure made of stars that wrap around the Milky Way galaxy in an orbit that nearly crosses the galactic poles. It consists of tidally stripped stars from the Sagittarius Dwarf Elliptical Galaxy, resulting from the process of merging with the Milky Way over a period ...