|NGC 4676A / 4676B|
The Mice Galaxies, NGC 4676A (right)/NGC 4676B (left)
|Observation data (J2000 epoch)|
|Right ascension||12h 46m 10.1s / 12h 46m 11.2s|
|Declination||+30° 43′ 55″ / +30° 43′ 22″|
|Redshift||6613 ± 8 / 6607 ± 7 km/s|
|Distance||290 Mly (89 Mpc)|
|Apparent magnitude (V)||14.7 / 14.4|
|Type||Irr / SB(s)0/a pec|
|Apparent size (V)||2′.3 × 0′.7 / 2′.2 × 0′.8|
|Notable features||Interacting galaxies|
PGC 43062 / 43065, Arp 242
NGC 4676, or the Mice Galaxies, are two spiral galaxies in the constellation Coma Berenices. About 290 million light-years away, they began the process of colliding and merging about 290 million years ago. Their name refers to the long tails produced by tidal action—the relative difference between gravitational pulls on the near and far parts of each galaxy—known here as a galactic tide. It is a possibility that both galaxies, which are members of the Coma cluster, have experienced collision, and will continue colliding until they coalesce.
The colors of the galaxy 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. NGC 4676B has a yellowish core and two arcs; arm remnants underneath are bluish as well.
- "NASA/IPAC Extragalactic Database". Results for NGC 4676A / 4676B. Retrieved 2006-11-21.
- Chien, Li-Hsin; Barnes, Joshua E.; Kewley, Lisa J.; Chambers, Kenneth, C. (May 2007). "Multiobject Spectroscopy of Young Star Clusters in NGC 4676". The Astrophysical Journal. 660 (2): L105–L108. arXiv: . Bibcode:2007ApJ...660L.105C. doi:10.1086/518215.
- "Hubble's New Camera Delivers Breathtaking Views of the Universe". HubbleSite. 2002-04-30. Retrieved 2009-05-07.
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