Astronomy:NGC 1268

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NGC 1268
NGC 1268 imaged by the Euclid Space Telescope
Observation data (J2000 epoch)
ConstellationPerseus
Right ascension 03h 18m 45.1985s[1]
Declination+41° 29′ 19.300″[1]
Redshift0.010748±0.000007[1][1]
Helio radial velocity3,222±2 km/s[1]
Distance147.3 ± 10.3 Mly (45.15 ± 3.17 Mpc)[1]
Group or clusterPerseus Cluster
Apparent magnitude (V)14.2[1]
Characteristics
TypeSAB(rs)b[1]
Size~55,400 ly (16.98 kpc) (estimated)[1]
Apparent size (V)1.0′ × 0.6′[1]
Other designations
UGC 2658, MCG+07-07-056, PGC 12332[1]

NGC 1268 is a spiral galaxy located about 147 million light-years away[2] in the constellation Perseus.[3] It was discovered by astronomer Heinrich d'Arrest on February 14, 1863.[4] NGC 1268 is a member of the Perseus Cluster[5][4] and appears to show signs of distortion in the form of bridges.[5] These features may be the result of a strong interaction with NGC 1267.[5][4]

Supernova

One supernova has been observed in NGC 1268. SN 2008fg (Type Ia, mag. 18.8) was discovered by the Lick Observatory Supernova Search (LOSS) on August 30, 2008.[6][7]

See also

References

Template:NGC objects:1000-1499

Coordinates: Sky map 03h 18m 45.1985s, +41° 29′ 19.300″