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  2. NGC 2 - Wikipedia

    en.wikipedia.org/wiki/NGC_2

    NGC 1 and NGC 2 as an optical double. NGC 2 is located about 345 million light-years from the Solar System, with a magnitude of +14.2, while the distance to NGC 1 is 210 million light-years. Although visually close in the sky, NGC 1 and NGC 2 are at very different distances; were they stars, they would be referred to as an "optical double" as ...

  3. Messier 2 - Wikipedia

    en.wikipedia.org/wiki/Messier_2

    Messier 2 or M2 (also designated NGC 7089) is a globular cluster in the constellation Aquarius, five degrees north of the star Beta Aquarii. It was discovered by Jean-Dominique Maraldi in 1746, and is one of the largest known globular clusters.

  4. List of NGC objects (1–1000) - Wikipedia

    en.wikipedia.org/wiki/List_of_NGC_objects_(1–1000)

    This is a list of NGC objects 1–1000 from the New General Catalogue (NGC). The astronomical catalogue is composed mainly of star clusters , nebulae , and galaxies . Other objects in the catalogue can be found in the other subpages of the list of NGC objects .

  5. NGC 2359 - Wikipedia

    en.wikipedia.org/wiki/NGC_2359

    NGC 2359 (also known as Thor's Helmet) is an emission nebula [3] in the constellation Canis Major. The nebula is approximately 3,670 parsecs (11.96 thousand light years) away and 30 light-years in size. The central star is the Wolf-Rayet star WR7, an extremely hot star thought to be in a brief pre-supernova stage of evolution.

  6. Mayall II - Wikipedia

    en.wikipedia.org/wiki/Mayall_II

    It is located 130,000 light-years (40 kpc) [3] from the Andromeda Galaxy's galactic core, and is the brightest [3] (by absolute magnitude) globular cluster in the Local Group, with an absolute visual magnitude of −10.94 and the luminosity of 2 million Suns. [4] It has an apparent magnitude of 13.81 in V band.

  7. Mice Galaxies - Wikipedia

    en.wikipedia.org/wiki/Mice_Galaxies

    NGC 4676, or the Mice Galaxies, are two spiral galaxies in the constellation Coma Berenices. About 290 million light-years distant, [ 2 ] they have begun the process of colliding and merging. Their "mice" name refers to the long tails produced by tidal action —the relative difference between gravitational pulls on the near and far parts of ...

  8. Messier 35 - Wikipedia

    en.wikipedia.org/wiki/Messier_35

    Messier 35 or M35, also known as NGC 2168 or the Shoe-Buckle Cluster, is a relatively close open cluster of stars in the west of Gemini, at about the declination of the Sun when the latter is at June solstice. [a] It was discovered by Philippe Loys de Chéseaux around 1745 and independently discovered by John Bevis before 1750. [3]

  9. Messier 47 - Wikipedia

    en.wikipedia.org/wiki/Messier_47

    Messier 47 (M47 or NGC 2422) and also known as NGC 2478 [3] is an open cluster in the mildly southern constellation of Puppis. It was discovered by Giovanni Batista Hodierna before 1654 and in his then keynote work re-discovered by Charles Messier on 1771. [a] It was also independently discovered by Caroline Herschel.

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