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  2. Ultra diffuse galaxy - Wikipedia

    en.wikipedia.org/wiki/Ultra_diffuse_galaxy

    NGC 1052-DF2, an ultra diffuse galaxy. An ultra diffuse galaxy (UDG), or dark galaxy, [1] is an extremely low luminosity galaxy, the first example of which was discovered in the nearby Virgo Cluster by Allan Sandage and Bruno Binggeli in 1984. [a] These galaxies have been studied for many years prior to their renaming in 2015. Their lack of ...

  3. Dark galaxy - Wikipedia

    en.wikipedia.org/wiki/Dark_galaxy

    A dark galaxy is a hypothesized galaxy with no (or very few) stars. They received their name because they have no visible stars but may be detectable if they contain significant amounts of gas. Astronomers have long theorized the existence of dark galaxies, but there are no confirmed examples to date. [1]

  4. Sombrero Galaxy - Wikipedia

    en.wikipedia.org/wiki/Sombrero_Galaxy

    The dark dust lane and the bulge give it the appearance of a sombrero hat (thus the name). Astronomers initially thought the halo was small and light, indicative of a spiral galaxy; but the Spitzer Space Telescope found that the halo was significantly larger and more massive than previously thought, indicative of a giant elliptical galaxy. [7]

  5. Hubble Ultra-Deep Field - Wikipedia

    en.wikipedia.org/wiki/Hubble_Ultra-Deep_Field

    The Hubble Ultra-Deep Field (HUDF) is a deep-field image of a small region of space in the constellation Fornax, containing an estimated 10,000 galaxies.The original data for the image was collected by the Hubble Space Telescope from September 2003 to January 2004 and the first version of the image was released on March 9, 2004. [1]

  6. GS-NDG-9422 - Wikipedia

    en.wikipedia.org/wiki/GS-NDG-9422

    GS-NDG-9422 is a nebular dominated galaxy in the constellation Fornax that was discovered by NASA’s James Webb Space Telescope. [ 1 ] [ 2 ] [ 3 ] Scientists assume that the galaxy's light comes mostly from superheated gas (more than 80 000 degrees Celsius).

  7. MACS J0416.1-2403 - Wikipedia

    en.wikipedia.org/wiki/MACS_J0416.1-2403

    MACS J0416.1-2403 or MACS0416 abbreviated, is a cluster of galaxies at a redshift of z=0.397 with a mass 160 trillion times the mass of the Sun inside 200 kpc (650 kly).Its mass extends out to a radius of 950 kpc (3,100 kly) and was measured as 1.15 × 10 15 solar masses. [2]

  8. Zooming In on the Andromeda Galaxy - Wikipedia

    en.wikipedia.org/wiki/Zooming_in_on_the...

    [7] [9] [10] In the bottom-left of the image is the galaxy's nucleus, and dust lanes are also visible. [11] Several other deep-space objects are visible in the image, including background galaxies. Stars within the Milky Way are also visible, and are typically larger than stars within the Andromeda Galaxy. [12] [13]

  9. Webb's First Deep Field - Wikipedia

    en.wikipedia.org/wiki/Webb's_First_Deep_Field

    The deep-field photograph, which covers a tiny area of sky visible from the Southern Hemisphere, is centered on SMACS 0723, a galaxy cluster in the constellation of Volans. Thousands of galaxies are visible in the image, some as old as 13 billion years. [1] It is the highest-resolution image of the early universe ever taken.

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