NGC 4330

Galaxy in the constellation Virgo From Wikipedia, the free encyclopedia

NGC 4330 is a spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 1898 ± 24 km/s, which corresponds to a Hubble distance of 27.99 ± 1.99 Mpc (~112 million light-years).[1] However, a dozen non-redshift measurements give a much closer distance of 19.642 ± 1.559 Mpc (~64.1 million light-years).[2] The galaxy was discovered by Irish engineer Bindon Stoney on 14 April 1852.[3]

Right ascension12h 23m 17.1775s[1]
Declination+11° 22 04.990[1]
Redshift0.005214[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 4330
NGC 4330 imaged by SDSS
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 23m 17.1775s[1]
Declination+11° 22 04.990[1]
Redshift0.005214[1]
Heliocentric radial velocity1563 ± 3 km/s[1]
Distance91.3 ± 6.5 Mly (27.99 ± 1.99 Mpc)[1]
Group or clusterM87 group (LGG 289)
Apparent magnitude (V)12.4[1]
Characteristics
TypeScd?[1]
Size~105,800 ly (32.43 kpc) (estimated)[1]
Apparent size (V)4.5′ × 0.9′[1] 4.5' x 0.9'[1]
Other designations
IRAS 12207+1138, 2MASX J12231724+1122047, UGC 7456, MCG +02-32-020, PGC 40201, CGCG 070-039, VCC 630[1]
Close

One supernova has been observed in NGC 4330: SN 2024phz (Type II, mag. 17.669) was discovered by ATLAS on 11 July 2024.[4]

M87 Group and Virgo Cluster

According to A.M. Garcia, NGC 4330 is a member of the M87 group (also known as LGG 289). This group contains at least 96 members.[5]

NGC 4330 is also listed as catalog number VCC 0630, a member of the Virgo Cluster.[6]

See also

References

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