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NGC 3414

Galaxy in the constellation Leo Minor From Wikipedia, the free encyclopedia

NGC 3414 is a lenticular galaxy in the constellation Leo Minor.[1] It was discovered by German-British astronomer William Herschel on April 11, 1785.[6] It is the central galaxy of a rich galaxy group.[4] Two galaxies, NGC 3418 and UGC 5958, have similar redshifts and are within 800,000 light-years (250 kiloparsecs) of NGC 3414.[7] It is a member of the NGC 3504 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.[8]

Quick facts Observation data (J2000 epoch), Constellation ...
NGC 3414
NGC 3414
legacy surveys image of NGC 3414 (bottom) and NGC 3418 (spiral galaxy at the top)
Observation data (J2000 epoch)
ConstellationLeo Minor[1]
Right ascension10h 51m 16.242s[2]
Declination+27° 58 29.88[2]
Redshift0.00485[3]
Heliocentric radial velocity1450 ± 55 km/s[3]
Distance77 Mly (23.5 Mpc)[4]
Apparent magnitude (V)11.09[5]
Apparent magnitude (B)12.06[5]
Characteristics
TypeS0pec[4]
Apparent size (V)3.5 × 2.6[1]
Other designations
Arp 162, UGC 5959, MCG +05-26-021, PGC 32533[3]
Close

It has a peculiar morphology, and is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 162.[3] The outer disc is nearly face-on, and the inner disk has a higher ellipticity and perhaps a central bar.[4] There is a radio source that is powered by a central active galactic nucleus.[7]

LDC 763 Galaxy group

NGC 3414 is the central member of the LDC 763 galaxy group, which also includes the neighboring galaxies NGC 3418 and UGC 5958.[9]

See also

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