Astronomy:NGC 1268

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Short description: Spiral galaxy in the constellation Perseus
NGC 1268
SDSS NGC 1268.jpg
SDSS image of NGC 1268.
Observation data (J2000 epoch)
ConstellationPerseus
Right ascension 03h 18m 45.1s[1]
Declination41° 29′ 19″[1]
Redshift0.010884[1]
Helio radial velocity3263 km/s[1]
Distance138 Mly (42.4 Mpc)[1]
Group or clusterPerseus Cluster
Apparent magnitude (V)14.2[1]
Characteristics
TypeSAB(rs)b[1]
Size~46,300 ly (14.20 kpc) (estimated)[1]
Apparent size (V)1.0 x 0.6[1]
Other designations
CGCG 540-93, MCG 7-7-56, PGC 12332, UGC 2658[1]

NGC 1268 is a spiral galaxy located about 140 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]

On August 30, 2008, a type Ia supernova designated as SN 2008fg was discovered in NGC 1268.[6][7][8]

See also

References

External links

Coordinates: Sky map 03h 18m 45.1s, +41° 29′ 19″