CEERS-2112
| CEERS-2112 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major/Boötes |
| Right ascension | 14h 19m 55.18s |
| Declination | 52° 59′ 31.1″ |
| Redshift | 3.03 |
| Heliocentric radial velocity | 986,317 km/h (612,869 mph) |
| Galactocentric velocity | 986,440 km/h (612,950 mph) |
| Distance | 11.7 billion ly (3.6 billion pc) (light travel distance) ~20 billion ly (6.1 billion pc) (comoving distance) |
| Characteristics | |
| Type | SBbc |
| Mass | 3.9×109 M☉ |
| Size | 30 kly (9.2 kpc) |
| Apparent size (V) | 0.009 x 0.005 moa |
| Other designations | |
| CANDELS J141955.18+525931.0, SYM2017 30172 | |
CEERS-2112 is the most distant barred spiral galaxy observed as of 2023. The light observed from the galaxy was emitted when the universe was only 2.1 billion years old. It was determined to be similar in mass to the Milky Way.