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(Top)
 


1 See also  





2 References  





3 External links  














NGC 18






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NGC 18


Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus[1]
Right ascension 00h09m23s[1]
Declination +27° 43′ 56[1]
Apparent magnitude (V) 14[1]
Other designations

Pul-3 10207/10208[2][3]

Database references
SIMBADPul-3 10207
Pul-3 10208

NGC 18 is a double star system located in the constellation of Pegasus.[1] It was first recorded by Herman Schultz on 15 October 1866. It was looked for but not found by Édouard Stephan on 2 October 1882. It was independently observed by Guillaume Bigourdan in November 1886.[1]

Both stars are 2528±20 light-years away, and based on this distance have a minimum separation of approximately 2,700 astronomical units, an unusually wide separation for a binary system.

See also

[edit]

References

[edit]
  1. ^ a b c d e f Seligman, Courtney (March 2010). "NGC Objects: NGC 1 - 49". Celestial Atlas. Retrieved 27 October 2010.
  • ^ "Pul-3 10207". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 31 January 2018.
  • ^ "Pul-3 10208". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 31 January 2018.
  • [edit]
    Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_18&oldid=1116346519"

    Categories: 
    Pegasus (constellation)
    Double stars
    NGC objects
    Astronomical objects discovered in 1866
    Hidden categories: 
    Articles with short description
    Short description is different from Wikidata
    Use dmy dates from December 2019
    Commons category link from Wikidata
     



    This page was last edited on 16 October 2022, at 03:15 (UTC).

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