NGC 18

Double star system in the constellation of Pegasus From Wikipedia, the free encyclopedia

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]

Quick facts Constellation, Right ascension ...
NGC 18

Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus[1]
Right ascension 00h 09m 23.1s[1]
Declination +27° 43 55[1]
Apparent magnitude (V) 14[1]
Other designations
Pul-3 10207/10208[2][3]
Database references
SIMBADPul-3 10207
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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.[citation needed]

See also

References

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