| IC 2006 | |
|---|---|
| IC 2006, imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 54m 28.427s [1] |
| Declination | −35° 58′ 01.75″ [1] |
| Redshift | 0.004610 [2] |
| Heliocentric radial velocity | 1382 [2] |
| Distance | 65.36 ± 0.46 Mly (20.04 ± 0.14 Mpc) [3] |
| Group or cluster | Fornax Cluster [3] |
| Apparent magnitude (B) | 12.39 [4] |
| Characteristics | |
| Type | E1 [5] |
| Size | 35 000 light-years in diameter |
| Apparent size (V) | 2.1′ × 1.8′ [2] |
| Notable features | Early-type galaxy |
| Other designations | |
| AM 0532-360, MGC-06-09-037, PGC 14077 | |
IC 2006 is an elliptical galaxy in the constellation Eridanus. The galaxy was discovered on 3 October 1897 by the American astronomer Lewis A. Swift. [6] It is estimated to be around 60 to 70 million light years (20 megaparsecs) away, [2] in the Fornax Cluster. [3] The galaxy is one of the smaller in the Fornax cluster, with a diameter of only 35 000 light-years.
IC 2006 is an early-type galaxy with a Hubble classification of E1, [5] but has also been listed as a lenticular galaxy with a morphological type of SA0−. [2] Despite their name, early-type galaxies are much older than spiral galaxies, and mostly comprise old, red-colored stars. Very little star formation occurs in these galaxies; the lack of star formation in elliptical galaxies appears to start at the center and then slowly propagates outward. [7] Its age is estimated to be 8.1 ± 1.7 billion years. [8]
An image taken by the Hubble Space Telescope in 2015 shows a characteristically smooth profile, with no spiral arms. [9] However, IC 2006 has a ring surrounding it. The ring appears to rotate in a direction opposite to the rest of the body, but this may be explained by a polar ring with an elliptical shape. [10]