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NGC 4458
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NGC 4458
The elliptical galaxy NGC 4458 as imaged by the SDSS.
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 28m 57.5s[1]
Declination13° 14′ 31″[1]
Redshift0.002258/677 km/s[1]
Distance54,801,600 ly
Group or clusterVirgo Cluster
Apparent magnitude (V)12.93 [1]
Characteristics
TypeE0 [1]
Mass~1.07×1010[2] M
Size~ 29,000 ly (estimated)[1]
Apparent size (V)1.7 x 1.6[1]
Other designations
CGCG 70-114, MCG 2-32-82, PGC 41095, UGC 7610, VCC 1146[1]

NGC 4458 is an elliptical galaxy located about 54 million light-years away[3][4] in the constellation of Virgo.[5] It was discovered by astronomer William Herschel on April 12, 1784.[6] NGC 4458 is a member of Markarian's Chain which is part of the Virgo Cluster.[7] It is in a pair with the galaxy NGC 4461.[8] NGC 4458 and NGC 4461 are interacting with each other.[9]

NGC 4458 may have a supermassive black hole with an estimated mass of 200 million Suns (2×108 M☉).[2]

Nuclear disk

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NGC 4458 has an edge-on nuclear disk which is estimated to be about 6 billion years old.[10] The disk likely formed from the merger of a gas-rich galaxy and has been found to have "similar properties to the decoupled cores of bright ellipticals".[11][12]

Counter-rotating core

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Using Hubble images, it has been determined that NGC 4458 has a counter-rotating core.[9]

Metallicity

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NGC 4458 has a low metal content but has an overabundance of the element iron.[9]

See also

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References

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