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Canis Major Dwarf Galaxy — 5,000 light years 5 × 10 19 meters Canes Venatici I — 6,500 light years 6.5 × 10 19 meters Small Magellanic Cloud: 3.5 × 10 19 meters 7,000 light years 7 × 10 19 meters Sagittarius Dwarf Galaxy: 10 19 meters 10,000 light years 10 20 meters Large Magellanic Cloud: 7.5 × 10 19 meters 14,000 light years 1.4 × ...
In July 2020, after a 20-year-long survey, astrophysicists of the Sloan Digital Sky Survey published the largest, most detailed 3D map of the universe so far, filled a gap of 11 billion years in its expansion history, and provided data which supports the theory of a flat geometry of the universe and confirms that different regions seem to be ...
The term "The Local Group" was introduced by Edwin Hubble in Chapter VI of his 1936 book The Realm of the Nebulae. [11] There, he described it as "a typical small group of nebulae which is isolated in the general field" and delineated, by decreasing luminosity, its members to be M31, Milky Way, M33, Large Magellanic Cloud, Small Magellanic Cloud, M32, NGC 205, NGC 6822, NGC 185, IC 1613 and ...
Additionally, most of the spacecraft included with Celestia 1.6.3 use outdated or low-quality models, such as the stock Mir model which is very basic and barely detailed, and the stock ISS model which hasn't had an update since around 2007, meaning it is missing a lot of modules that have been added to the ISS since then.
ZFOURGE or the FourStar Galaxy Evolution Survey is a large and deep medium-band imaging survey which aims to establish an observational benchmark of galaxy properties at redshift z > 1. The survey is using near-infrared FOURSTAR instrument on the Magellan Telescopes , surveying in all three HST legacy fields: COSMOS, CDFS, and UDS.
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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).
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