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  2. Andromeda Galaxy - Wikipedia

    en.wikipedia.org/wiki/Andromeda_Galaxy

    The Andromeda Galaxy is known to harbor a dense and compact star cluster at its very center, similar to our own galaxy. A large telescope creates a visual impression of a star embedded in the more diffuse surrounding bulge. In 1991, the Hubble Space Telescope was used to image the Andromeda Galaxy's inner nucleus.

  3. NGC 828 - Wikipedia

    en.wikipedia.org/wiki/NGC_828

    NGC 828 is a spiral galaxy in the constellation of Andromeda. Its velocity with respect to the cosmic microwave background is 5118 ± 17 km/s, which corresponds to a Hubble distance of 75.49 ± 5.29 Mpc (∼246 million light-years). [1] It was discovered by German-British astronomer William Herschel on 18 October 1786.

  4. NGC 752 - Wikipedia

    en.wikipedia.org/wiki/NGC_752

    NGC 752. NGC 752 (also known as Caldwell 28) is an open cluster in the constellation Andromeda. The cluster was discovered by Caroline Herschel in 1783 and cataloged by her brother William Herschel in 1786, although an object that may have been NGC 752 was described by Giovanni Batista Hodierna before 1654. [4]

  5. Andromeda–Milky Way collision - Wikipedia

    en.wikipedia.org/wiki/Andromeda–Milky_Way...

    The Andromeda–Milky Way collision is a galactic collision predicted to occur in about 4.5 billion years between the two largest galaxies in the Local Group —the Milky Way (which contains the Solar System and Earth) and the Andromeda Galaxy. [1][2][3][4][5] The stars involved are sufficiently far apart that it is improbable that any of them ...

  6. NGC 67 - Wikipedia

    en.wikipedia.org/wiki/NGC_67

    NGC 67. NGC 67 is an elliptical galaxy located in the constellation Andromeda that was discovered on October 7, 1855, by R. J. Mitchell, who described it as "extremely faint, very small, round". The galaxy belongs to the NGC 68 group, which also contains the galaxies NGC 68, NGC 69, NGC 70, NGC 71, NGC 72, and possibly NGC 74.

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

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

    August 20, 2024 at 5:02 PM. Our Galaxy Might Not Be Doomed After AllNASA; ESA; Z. Levay and R. van der Marel, STScI; T. Hallas; and A. Mellinger. For nearly two decades, astronomers have been ...

  8. NGC 206 - Wikipedia

    en.wikipedia.org/wiki/NGC_206

    NGC 206 is the richest and most conspicuous star cloud in the Andromeda Galaxy, and is one of the largest and brightest star-forming regions in the Local Group. [2] It contains more than 300 stars brighter than M b =−3.6. [3] It was originally identified by Edwin Hubble as a star cluster but today, due to its size, it is classified as an OB ...

  9. NGC 80 - Wikipedia

    en.wikipedia.org/wiki/NGC_80

    Size. 166,900 ly (51,160 pc) [2] Apparent size (V) 2.2 ′ × 2.002 ′ [2] Other designations. UGC 203, MCG +04-02-004, PGC 1351 [4] NGC 80 is a lenticular galaxy located in the constellation Andromeda. It is currently interacting with two other barred spiral galaxies NGC 47 and NGC 68, and was discovered on August 17, 1828 by John Herschel.

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