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Magellanic spiral galaxy in the constellation Draco From Wikipedia, the free encyclopedia
UGC 9391 is a Magellanic spiral galaxy in constellation Draco. 130 million light years from Earth, it is not a member of any group of galaxies, and is moving away from the Earth at 1939 km/s.[2]
UGC 9391 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Draco |
Right ascension | 14h 34m 37.013s[1] |
Declination | 59° 20m 16.174s[1] |
Redshift | 0.00649[1] |
Heliocentric radial velocity | 1,939 km/s[2] |
Distance | 78.8 Mly (24.15 Mpc)[3] |
Apparent magnitude (B) | 15.5[2] |
Characteristics | |
Type | SBdm[3] |
Apparent size (V) | 1.85′ × 1.85′[2] |
Other designations | |
UGC 9391, MCG +10-21-011, PGC 52091[2] |
In 2003, a supernova catalogued as SN 2003du was detected within the galaxy, with an apparent magnitude of 15.9.[4]
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