NGC 1090

Galaxy in the constellation Cetus From Wikipedia, the free encyclopedia

NGC 1090 is a barred spiral galaxy located in the constellation Cetus.

Right ascension02h 46m 33.9s[1]
Declination−00° 14 49[1]
Redshift2760 ± 4 km/s[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 1090
NGC 1090 imaged by SDSS
Observation data (J2000 epoch)
ConstellationCetus
Right ascension02h 46m 33.9s[1]
Declination−00° 14 49[1]
Redshift2760 ± 4 km/s[1]
Distance124 million light-years[2]
Apparent magnitude (V)12.5[1]
Characteristics
TypeSB(rs)bc[1]
Apparent size (V)4.0 × 1.7[1]
Other designations
UGC 2247,[1] PGC 10507[1]
Close

NGC 1090 has a pseudo inner ring. The disc has a very low surface brightness.

NGC 1090 is not part of a galaxy group, even though it appears close to NGC 1087, M77 (NGC 1068), NGC 1055, NGC 1073, and five other small irregular galaxies.

The distance to NGC 1090 is approximately 124 million light years and its diameter is about 144,000 light years.[2]

Supernovae

Two supernovae have been observed in NGC 1090:

References

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