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  2. Small Magellanic Cloud - Wikipedia

    en.wikipedia.org/wiki/Small_Magellanic_Cloud

    The Small Magellanic Cloud (SMC) is a dwarf galaxy near the Milky Way. [5] Classified as a dwarf irregular galaxy , the SMC has a D 25 isophotal diameter of about 5.78 kiloparsecs (18,900 light-years), [ 1 ] [ 3 ] and contains several hundred million stars. [ 5 ]

  3. Magellanic Clouds - Wikipedia

    en.wikipedia.org/wiki/Magellanic_Clouds

    The Large Magellanic Cloud and its neighbour and relative, the Small Magellanic Cloud, are conspicuous objects in the southern hemisphere, looking like separated pieces of the Milky Way to the naked eye. Roughly 21° apart in the night sky, the true distance between them is roughly 75,000 light-years.

  4. NGC 121 - Wikipedia

    en.wikipedia.org/wiki/NGC_121

    The compiler of the New General Catalogue, Danish astronomer John Louis Emil Dreyer, described this object as "pretty bright, pretty small, little extended, very gradually brighter middle". [6] The cluster is located at a distance of around 200,000 light-years (60 kpc ) from the Sun. [ 1 ]

  5. Cosmic distance ladder - Wikipedia

    en.wikipedia.org/wiki/Cosmic_distance_ladder

    This makes it feasible to use them as indicators of distance. Recently, they have been used to give direct distance estimates to the Large Magellanic Cloud (LMC), Small Magellanic Cloud (SMC), Andromeda Galaxy and Triangulum Galaxy. Eclipsing binaries offer a direct method to gauge the distance to galaxies to a new improved 5% level of accuracy ...

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

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

    (Located in Small Magellanic Cloud) Open cluster: Tucana: 00 h 51 m 14.1 s: −73° 09′ 42″ 12.1 291: Barred spiral galaxy: Cetus: 00 h 53 m 29.8 s: −08° 46′ 04″ 14 292: Small Magellanic Cloud Irregular galaxy: Tucana: 00 h 52 m 38.0 s: −72° 48′ 01″ 2.8 293: Spiral galaxy: Cetus: 00 h 54 m 16.0 s: −07° 14′ 09″ 14 294 ...

  7. NGC 330 - Wikipedia

    en.wikipedia.org/wiki/NGC_330

    NGC 330 is an open cluster in the Small Magellanic Cloud.It is located in the constellation Tucana.It was discovered on 1 August 1826 by James Dunlop.It was described by Dreyer as "a globular cluster, very bright, small, a little extended, stars from 13th to 15th magnitude."

  8. In a first, a newborn star's spinning disk is seen in ... - AOL

    www.aol.com/news/first-newborn-stars-spinning...

    The Large Magellanic Cloud is considered a satellite galaxy of the sprawling Milky Way, as is another galaxy called the Small Magellanic Cloud. Both are smaller than our galaxy and offer different ...

  9. Orders of magnitude (length) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude_(length)

    1.7 Zm – 179,000 light-years – distance to the Large Magellanic Cloud, largest satellite galaxy of the Milky Way <1.9 Zm – <200,000 light-years – revised estimated diameter of the disc of the Milky Way Galaxy. The size was previously thought to be half of this. 2.0 Zm – 210,000 light-years – distance to the Small Magellanic Cloud

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