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  2. Ring galaxy - Wikipedia

    en.wikipedia.org/wiki/Ring_galaxy

    A ring galaxy is a galaxy with a circle-like appearance. Hoag's Object, discovered by Arthur Hoag in 1950, is an example of a ring galaxy. [1] The ring contains many massive, relatively young blue stars, which are extremely bright. The central region contains relatively little luminous matter. Some astronomers believe that ring galaxies are ...

  3. Hoag's Object - Wikipedia

    en.wikipedia.org/wiki/Hoag's_Object

    Many of the galaxy's details remain mysterious, foremost of which is how it formed. So-called "classic" ring galaxies are generally formed by the collision of a small galaxy with a larger disk-shaped galaxy, producing a density wave in the disk that leads to a characteristic ring-like appearance.

  4. List of ring galaxies - Wikipedia

    en.wikipedia.org/wiki/List_of_ring_galaxies

    The cartwheel galaxy, galaxy pair AM 2026-424, and Arp 147 are all examples of ring galaxies believed to be formed from this process. In pass-through galactic collisions, an often smaller galaxy will pass through the disc of an often larger spiral, causing an outward push of the arms, as if dropping a rock into a pond of still water.

  5. Cartwheel Galaxy - Wikipedia

    en.wikipedia.org/wiki/Cartwheel_Galaxy

    The Cartwheel Galaxy (also known as ESO 350-40 or PGC 2248) is a lenticular ring galaxy about 500 million light-years away in the constellation Sculptor. [1] It has a D 25 isophotal diameter of 44.23 kiloparsecs (144,300 light-years), and a mass of about 2.9–4.8 × 10 9 solar masses; its outer ring has a circular velocity of 217 km/s.

  6. AM 0644-741 - Wikipedia

    en.wikipedia.org/wiki/AM_0644-741

    The yellowish nucleus was once the center of a normal spiral galaxy, and the ring which currently surrounds the center is 150,000 light years in diameter. [2] The ring is theorized to have formed by a collision with another galaxy, which triggered a gravitational disruption that caused dust in the galaxy to condense and form stars, which forced it to then expand away from the galaxy and create ...

  7. NGC 2445 - Wikipedia

    en.wikipedia.org/wiki/NGC_2445

    NGC 2445 is characterised by its distorted shape and star formation which is the result of the collision with another galaxy, NGC 2444. NGC 2444 has pulled gas away from NGC 2445 and as a result a bridge of young blue stars has formed between the two galaxies that gives the latter a triangular shape. [3]

  8. Our Galaxy Might Not Be Doomed After All - AOL

    www.aol.com/well-50-50-galaxy-collide-185300912.html

    Scientists say there's a 50/50 chance that our Milky Way galaxy will ... The authors behind this new study were the first to calculate the probability of a Milky Way-Andromeda collision ...

  9. LEDA 1000714 - Wikipedia

    en.wikipedia.org/wiki/LEDA_1000714

    LEDA 1000714 [3] is a ring galaxy in the constellation Crater.LEDA 1000714 is one of a very rare group of galaxies called Hoag-type galaxies, [3] named after the prototype, Hoag's Object – it is estimated that roughly 0.1% of all galaxies are this type.