NGC 5162 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 13h 29m 25.9296s[1] |
Declination | +11° 00′ 28.534″[1] |
Redshift | 0.022799[1] |
Heliocentric radial velocity | 6835 ± 1 km/s[1] |
Distance | 342.8 ± 24.0 Mly (105.09 ± 7.36 Mpc)[1] |
Apparent magnitude (V) | 13.0[1] |
Characteristics | |
Type | Scd?[1] |
Size | ~326,900 ly (100.22 kpc) (estimated)[1] |
Apparent size (V) | 2.7′ × 1.4′[1] |
Other designations | |
IRAS 13269+1115, 2MASX J13292596+1100285, NGC 5174, UGC 8475, MCG +02-34-018, PGC 47346, CGCG 072-087[1] |
NGC 5162 is a very large spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 7125 ± 20 km/s, which corresponds to a Hubble distance of 342.8 ± 24.0 Mly (105.09 ± 7.36 Mpc).[1] In addition, 11 non redshift measurements give a distance of 303.71 ± 12.41 Mly (93.118 ± 3.806 Mpc).[2] The galaxy was discovered by German-British astronomer William Herschel on 15 March 1784.[3] It was also observed by Lewis Swift on 19 April 1887, resulting in the galaxy being included twice in the New General Catalogue, as both NGC 5162 and NGC 5174.[3]
The SIMBAD database lists NGC 5162 as a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[4] NGC 5162 is a field galaxy, i.e. it does not belong to a larger galaxy group or cluster and hence is gravitationally alone.[5]
Two supernovae have been observed in NGC 5162. Kōichi Itagaki discovered SN 2007cd (type unknown, mag. 17.5) on 27 April 2007.[6] The Xingming Observatory Sky Survey discovered SN 2024aawh (type II, mag. 18.11) on 10 November 2024.[7]
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