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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, [3] the MilkyWay@home project aims to generate accurate three-dimensional dynamic models of stellar streams in the ...

  3. Gaia Sky - Wikipedia

    en.wikipedia.org/wiki/Gaia_Sky

    Gaia Sky is an open-source astronomy visualisation desktop and VR program with versions for Windows, Linux and macOS.It is created and developed by Toni Sagristà Sellés in the framework of ESA's Gaia mission to create a billion-star multi-dimensional map of our Milky Way Galaxy, in the Gaia group of the Astronomisches Rechen-Institut (ZAH, Universität Heidelberg).

  4. Thin disk - Wikipedia

    en.wikipedia.org/wiki/Thin_disk

    The Thin disk is shown in green. The thin disk is a structural component of spiral and S0-type galaxies, composed of stars, gas and dust. It is the main non-centre (e.g. galactic bulge) density, of such matter. That of the Milky Way is thought to have a scale height of around 300–400 parsecs (980–1,300 ly) in the vertical axis perpendicular ...

  5. Galactic disc - Wikipedia

    en.wikipedia.org/wiki/Galactic_disc

    A galactic disc (or galactic disk) is a component of disc galaxies, such as spiral galaxies like the Milky Way and lenticular galaxies. 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). The stellar population of galactic discs tend to exhibit ...

  6. Astropulse - Wikipedia

    en.wikipedia.org/wiki/Astropulse

    Astropulse searches for pulses with dispersion measures ranging from 50 pc/cm 3 to 800 pc/cm −3 (chirp rates of 7000 Hz to 400 Hz per microsecond), allowing detection of sources almost anywhere within the Milky Way. Project proponents believe that Astropulse will either detect exploding black holes, or establish a maximum rate of 5 × 10 − ...

  7. Voyager 1 - Wikipedia

    en.wikipedia.org/wiki/Voyager_1

    Communication system. [edit] The radio communication system of Voyager 1 was designed to be used up to and beyond the limits of the Solar System. It has a 3.7-metre (12 ft) diameter high-gain Cassegrain antenna to send and receive radio waves via the three Deep Space Network stations on the Earth. [ 21 ]

  8. Tianhe-2 - Wikipedia

    en.wikipedia.org/wiki/Tianhe-2

    Tianhe-2 or TH-2 (Chinese: 天河-2; pinyin: tiānhé-èr; lit. 'Heavenriver-2', i.e. ' Milky Way 2') is a 3.86- petaflop supercomputer located in the National Supercomputer Center in Guangzhou, China. [3] It was developed by a team of 1,300 scientists and engineers. It was the world's fastest supercomputer according to the TOP500 lists for ...

  9. The Milky Way Project - Wikipedia

    en.wikipedia.org/wiki/The_Milky_Way_Project

    The Milky Way Project. The Milky Way Project is a Zooniverse project whose main goal is to identify stellar-wind bubbles in the Milky Way Galaxy. Users classify sets of infrared images from the Spitzer Space Telescope and the Wide-field Infrared Survey Explorer (WISE). [1] Scientists believe bubbles in these images are the result of young ...