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| NGC 4676A / 4676B | |
|---|---|
.jpg) The Mice Galaxies, NGC 4676A (right) / NGC 4676B (left) | |
| Observation data (J2000epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 46m 10.1s /12h 46m 11.2s[1] |
| Declination | +30° 43′ 55″ / +30° 43′ 22″[1] |
| Redshift | 6613 ± 8 / 6607 ± 7 km/s[1] |
| Distance | 290 Mly (89 Mpc)[2] |
| Apparent magnitude (V) | 14.7 / 14.4[1] |
| Characteristics | |
| Type | Irr / SB(s)0/a pec[1] |
| Size | 760,000 ly (233 kpc) (estimated)[a] |
| Apparent size (V) | 2′.3 × 0′.7 / 2′.2 × 0′.8[1] |
| Notable features | Interacting galaxies |
| Other designations | |
| Mice Galaxies,[1]IC 819 / 820,[1]UGC 7938 / 7939,[1] PGC 43062 / 43065,[1]Arp 242[1] | |
NGC 4676, or theMice Galaxies, are twospiral galaxies in theconstellationComa Berenices. About 290 millionlight-years distant,[2] they have begun the process of colliding and merging. Their "mice" name refers to the long tails produced bytidal action—the relative difference between gravitational pulls on the near and far parts of each galaxy—known here as agalactic tide. It is a possibility that both galaxies, which are members of theComa Cluster,[3] have experienced collision, and will continue colliding until they coalesce.
The colors of the galaxies are peculiar. In NGC 4676A a core with some dark markings is surrounded by a bluish white remnant of spiral arms. The tail is unusual, starting out blue and terminating in a more yellowish color, despite the fact that the beginning of each arm in virtually every spiral galaxy starts yellow and terminates in a bluish color.[citation needed][clarification needed] NGC 4676B has a yellowish core and two arcs; arm remnants underneath are bluish as well.
The galaxies were photographed in 2002 by theHubble Space Telescope.[4] In the background of the Mice Galaxies, there are over 3000 galaxies, at distances up to 13 billion light-years.
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