because they can clearly see distant galaxies behind it. other large galaxies are present, such as the giant spiral NGC 1042. galaxies in the relatively nearby Universe (within 100 million light years), has found a unique galaxy in NGC 1052-DF2. Nearby to these galaxies are small, barely-visible ultra diffuse galaxies, known as NGC 1052-DF2 and NGC 1052-DF4 (or just DF2 and DF4 for short) which appear to be made of normal matter alone if they're at the distance of NGC 1052: 60 to 70 million light-years away. A different team claimed these galaxies belong to a closer foreground group, implying a typical dark matter density.
At the dawn of 2018, however, the controversy over the expanding Universe might threaten that picture. arXiv:1901.03711, with the earlier results from a competing team using MUSE superimposed in red. The results of Trujillo et al. of its gas) at a few percent the speed of light: thousands of km/s. Controversy continues By Emily Conover August 5, 2020. The ghostly object, catalogued as NGC 1052-DF2, doesn’t have a noticeable central region, or even spiral arms and a disk, typical features of a spiral galaxy. W.M. publication in 2018 announcing the discovery of DF2. Joined by DF4, these galaxies could solve an enormous cosmic puzzle.


Danieli, Van Dokkum and others, goes eight times deeper than previous observations. I have won numerous awards for science writing since 2008 for my blog, Opinions expressed by Forbes Contributors are their own.The Universe is out there, waiting for you to discover it. The zoom-in showsThe key advance was measuring their velocity dispersions, an achievement enabled by modern instrumentation.The Dragonfly telephoto array, which is optimized for finding extremely low-surface-brightnessThose measurements, combined with parent galaxy NGC 1052's distance, allowed reconstruction of their total masses.The KCWI spectrum of the galaxy DF2 (in black), as taken directly from the new paper atWith distances estimated at ~60-70 million light-years, their galactic properties indicate a dark matter-free composition.The galaxy NGC 1052-DF2 was imaged in great detail by the KCWI spectrograph instrument aboard theThis large, fuzzy-looking galaxy is so diffuse that astronomers call it a “see-through” galaxyThe ultra-diffuse galaxy KKS2000]04 (NGC1052-DF2), towards the constellation of Cetus, wasHubble measurements of the other galaxy, NGC 1052-DF4, The new data on galaxy NGC 1052-DF4, as taken with the Hubble Space Telescope by the team ofMany nearby galaxies, including all the galaxies of the local group (mostly clustered at the extremeIf these galaxies truly possess the sizes, distances, and velocity dispersions measured, they must be dark matter-free.I am a Ph.D. astrophysicist, author, and science communicator, who professes physics and astronomy at various colleges. I have won numerous awards for science writingI am a Ph.D. astrophysicist, author, and science communicator, who professes physics and astronomy at various colleges. This is the seventh Dark Matter in the city but the first focusing exclusively on Mexican cacao. Scientists understanding of dark matter and gravity could be completely wide of the mark, according to a new theory. Keck telescope on Mauna Kea, enabling scientists to detect the motions of stars and globular clusters inside the galaxy to unprecedented precisions. An evolved version of such objects, which ought to represent a clump of normal matter ejected from a host galaxy, could create a dark matter-free galaxy like DF2 and DF4 are suspected to be.

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