| IC 4026 | |
|---|---|
Sloan Digital Sky Survey image of IC 4026
| |
| Observation data | |
| Constellation | Coma Berenices |
| Right ascension | 195.0 degrees |
| Declination | 28.04 degrees |
| Redshift | 0.02727 |
| Heliocentric radial velocity | 8,196 km/s |
| Distance | 315 Mly (96.5 Mpc) |
| Grouporcluster | Coma Cluster |
| Apparent magnitude (V) | 14.63 |
| Surface brightness | 11.99 mag/arcsec |
| Characteristics | |
| Type | SB0 |
| Size | 70,000 ly |
| Other designations | |
| PGC 44749, CGCG 160-250, WBL 426-100, AGC 221386, UZC J130022.0+280250, NSA 104078, SDSS J130022.12+280249.2, 2MASX J13002215+2802495, [DZ2015] 703-29, MaNGA 01-456903, LEDA 44749 | |
IC 4026 is a type S0 lenticular galaxy with a bar[1] located in Coma Berenices.[2][3] It is located 315 million light-years away from the Solar System and has an approximate diameter of 70,000 light-years which is less the size of the Milky Way.[4] IC 4026 was discovered on May 11, 1896, by astronomer Hermann Kobold[5] and is a member of the Coma Cluster.[4][6][7] It has a surface brightness of 11.99 mag/arcsecs meaning it is a high surface brightness galaxy.[8]
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