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  2. Andromeda Galaxy - Wikipedia

    en.wikipedia.org/wiki/Andromeda_Galaxy

    The Andromeda Galaxy is a barred spiral galaxy and is the nearest major galaxy to the Milky Way. It was originally named the Andromeda Nebula and is cataloged as Messier 31, M31, and NGC 224. Andromeda has a D 25 isophotal diameter of about 46.56 kiloparsecs (152,000 light-years) and is approximately 765 kpc (2.5 million light-years) from Earth.

  3. Andromeda–Milky Way collision - Wikipedia

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

    This series of photo illustrations shows the predicted merger between the Milky Way galaxy and the neighboring Andromeda Galaxy. The Andromeda Galaxy is approaching the Milky Way at about 300 km/s (200 miles per second) as indicated by blueshift.

  4. List of Andromeda's satellite galaxies - Wikipedia

    en.wikipedia.org/wiki/List_of_Andromeda's...

    The Andromeda Galaxy (M31) has satellite galaxies just like the Milky Way. Orbiting M31 are at least 13 dwarf galaxies: the brightest and largest is M110, which can be seen with a basic telescope. The second-brightest and closest one to M31 is M32. The other galaxies are fainter, and were mostly discovered starting from the 1970s.

  5. List of nearest galaxies - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_galaxies

    List of nearest galaxies. This is a list of known galaxies within 3.8 megaparsecs (12.4 million light-years) of the Solar System, in ascending order of heliocentric distance, or the distance to the Sun. This encompasses about 50 major Local Group galaxies, and some that are members of neighboring galaxy groups, the M81 Group and the Centaurus A ...

  6. Andromeda (constellation) - Wikipedia

    en.wikipedia.org/wiki/Andromeda_(constellation)

    The constellation's most obvious deep-sky object is the naked-eye Andromeda Galaxy (M31, also called the Great Galaxy of Andromeda), the closest spiral galaxy to the Milky Way and one of the brightest Messier objects. Several fainter galaxies, including M31's companions M110 and M32, as well as the more distant NGC 891, lie within Andromeda.

  7. PA-99-N2 - Wikipedia

    en.wikipedia.org/wiki/PA-99-N2

    PA-99-N2 is a microlensing event detected in the direction of the Andromeda Galaxy in 1999. Explanations. One possibility for the event is that a star in the disk of M31 gravitationally lensed a red giant also in the disk. The lensing star would have a mass between 0.02 M ☉ and 3.6 M ☉ with the most likely value near 0.5 M ☉.

  8. Nu Andromedae - Wikipedia

    en.wikipedia.org/wiki/Nu_Andromedae

    Situated just over a degree to the west of this star is the Andromeda Galaxy. [12] Nu Andromedae is the prominent blue star in the upper right of this image. At the center is the Andromeda Galaxy. Nu Andromedae is spectroscopic binary [3] system with a nearly circular orbit that has a period of 4.2828 days. [5]

  9. Andromeda X - Wikipedia

    en.wikipedia.org/wiki/Andromeda_X

    Andromeda X (And 10) is a dwarf spheroidal galaxy about 2.9 million light-years away from the Sun in the constellation Andromeda. [1] Discovered in 2005 by Zucker et al., And X is a satellite galaxy of the Andromeda Galaxy (M31).

  10. Alpheratz - Wikipedia

    en.wikipedia.org/wiki/Alpheratz

    Andromeda constellation. α Andromedae, labeled Sirrah, is at the lower right of the constellation, bordering Pegasus. The location of α Andromedae in the sky is shown on the left. It can be seen by the naked eye and is theoretically visible at all latitudes north of 60° S.

  11. 14 Andromedae b - Wikipedia

    en.wikipedia.org/wiki/14_Andromedae_b

    14 Andromedae b (abbreviated 14 And b), formally named Spe / ˈ s p iː /, is an exoplanet approximately 249 light years away in the constellation of Andromeda. The 186-day period planet orbits about 83% the Earth-Sun distance from the giant star 14 Andromedae. It has a minimum mass 4.8 times the mass of Jupiter.