NGC 5112 | |
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![]() NGC 5112 imaged by theHubble Space Telescope | |
Observation data (J2000epoch) | |
Constellation | Canes Venatici |
Right ascension | 13h 21m 56.4s[1] |
Declination | +38° 44′ 05″[1] |
Redshift | 0.003219[1] |
Heliocentric radial velocity | 965 ± 9km/s[1] |
Distance | 62 ± 3 Mly (19.1 ± 1 Mpc)[2] |
Apparent magnitude (V) | 14.2[1] |
Characteristics | |
Type | SB(rs)cd[1] |
Apparent size (V) | 4.0′ × 2.8′[1] |
Other designations | |
IRAS 13196+3859,UGC 8403,MCG +07-28-003,PGC 46671,CGCG 218-005[1] |
NGC 5112 is abarred spiral galaxy in theconstellationCanes Venatici. It was discovered on 17 March 1787 byGerman-British astronomerWilliam Herschel.[3] This galaxy is in close physical proximity to the edge-on dwarf spiralNGC 5107.
On 4 March 2015, asupernova candidate was discovered in NGC 5112, and designatedPSN J13215756+3843229. Spectral analysis suggested that it was instead asupernova imposter, possibly an outburst from aluminous blue variable.[4]
According to A. M. Garcia, NGC 5112 is part of the NGC 5005group (also known asLGG 334). This group of galaxies contains at least 16 members. The other galaxies in the group are:NGC 4861,NGC 5002,NGC 5005,NGC 5014,NGC 5033,NGC 5107,IC 4182,IC 4213, UGC 8181, UGC 8246, UGC 8261, UGC 8303, UGC 8314, UGC 8315, and UGC 8323.[5]
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