Astronomy:NGC 4168

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NGC 4168
NGC 4168 with NGC 4165 (above, to the right) and NGC 4164 (to the right), imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension 12h 12m 17.2685s[1]
Declination+13° 12′ 18.701″[1]
Redshift0.007582±0.00000667[1]
Helio radial velocity2,273±2 km/s[1]
Distance98.35 ± 10.89 Mly (30.154 ± 3.338 Mpc)[1]
Group or clusterVirgo Cluster
Apparent magnitude (V)12.4g[1]
Characteristics
TypeE2[1]
Size~80,100 ly (24.56 kpc) (estimated)[1]
Apparent size (V)2.03′ × 1.58′[1]
Other designations
VCC 49, UGC 7203, MCG+02-31-046, PGC 38890[1]

NGC 4168 is an elliptical galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 2,609±24 km/s, which corresponds to a Hubble distance of 125.5 ± 8.9 Mly (38.48 ± 2.72 Mpc).[1] However, 13 non-redshift measurements give a closer mean distance of 98.35 ± 10.89 Mly (30.154 ± 3.338 Mpc).[2] It was discovered by German-British astronomer William Herschel on 8 April 1784.[3]

NGC 4168 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[4][5]

Virgo cluster

NGC 4168 is a member of the Virgo Cluster.[5][6]

Supernova

One supernova has been observed in NGC 4168:

  • SN 2026acd (Type Ia, mag. 18.876) was discovered by ATLAS on 14 January 2026.[7]

See also

References

Coordinates: Sky map 12h 12m 17.2685s, +13° 12′ 18.701″