Double star system in the constellation of Pegasus
NGC 18
Observation data Epoch J2000 Equinox J2000
Constellation
Pegasus[1]
Right ascension
00h 09m 23s[1]
Declination
+27° 43′ 56″[1]
Apparent magnitude (V)
14[1]
Other designations
Pul-3 10207/10208[2][3]
Database references
SIMBAD
Pul-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.
^ abcdefSeligman, 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.
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