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  2. Messier 100 - Wikipedia

    en.wikipedia.org/wiki/Messier_100

    Messier 100 (also known as NGC 4321 or the Mirror Galaxy) is a grand design intermediate spiral galaxy in the southern part of the mildly northern Coma Berenices. [5] It is one of the brightest and largest galaxies in the Virgo Cluster and is approximately 55 million light-years [ 3 ] from our galaxy , about 166,000 light-years in diameter.

  3. NGC 908 - Wikipedia

    en.wikipedia.org/wiki/NGC_908

    NGC 908 is an unbarred spiral galaxy in the constellation Cetus. It was discovered on 20 September 1786 by William Herschel. [3] This galaxy is 56 million light years away from Earth. It is the main galaxy in the NGC 908 group, which also includes NGC 899, NGC 907, and IC 223. [4] NGC 908 has vigorous star formation and is a starburst galaxy ...

  4. NGC 891 - Wikipedia

    en.wikipedia.org/wiki/NGC_891

    NGC 891 looks as the Milky Way would look like when viewed edge-on (some astronomers have even noted how similar to NGC 891 our galaxy looks as seen from the Southern Hemisphere [9]) and, in fact, both galaxies are considered very similar in terms of luminosity and size; [10] studies of the dynamics of its molecular hydrogen have also proven the likely presence of a central bar. [11]

  5. Galaxy - Wikipedia

    en.wikipedia.org/wiki/Galaxy

    Our own galaxy, the Milky Way, is a large disk-shaped barred-spiral galaxy [92] about 30 kiloparsecs in diameter and a kiloparsec thick. It contains about two hundred billion (2×10 11 ) [ 93 ] stars and has a total mass of about six hundred billion (6×10 11 ) times the mass of the Sun. [ 94 ]

  6. Messier 99 - Wikipedia

    en.wikipedia.org/wiki/Messier_99

    Coma Pinwheel Galaxy, Virgo Cluster Pinwheel, M99, NGC 4254, PGC 39578, UGC 7345 [9] Messier 99 or M99 , also known as NGC 4254 or St. Catherine's Wheel , is a grand design spiral galaxy in the northern constellation Coma Berenices approximately 15,000,000 parsecs (49,000,000 light-years ) from the Milky Way . [ 5 ]

  7. Messier 22 - Wikipedia

    en.wikipedia.org/wiki/Messier_22

    M22 is one of only four globulars of our galaxy [c] known to contain a planetary nebula (an expanding, glowing gas swell from a massive star, often a red giant). It was an object first noted of interest using the IRAS satellite by Fred Gillett and his associates in 1986, as a pointlike light source [ d ] [ 16 ] and its nature was found in 1989 ...

  8. NGC 1073 - Wikipedia

    en.wikipedia.org/wiki/NGC_1073

    NGC 1073 is a barred spiral galaxy in the constellation Cetus.The galaxy is estimated to be about 55 million light years from Earth, possess a disk spanning an estimated 80,000 light years in diameter, and likely contains a type of active core, called an HII nucleus.

  9. NGC 7331 - Wikipedia

    en.wikipedia.org/wiki/NGC_7331

    NGC 7331 is the brightest galaxy in the field of a visual grouping known as the NGC 7331 Group of galaxies. In fact, the other members of the group, NGC 7335 , NGC 7336 , NGC 7337 and NGC 7340 , lie far in the background at distances of approximately 300–350 million light years.

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