| UGC 11105 | |
|---|---|
.jpg)
Hubble Space Telescope image of UGC 11105 | |
| Observation data | |
| Constellation | Hercules |
| Right ascension | 271.1 degrees |
| Redshift | 0.007418 0.000013 |
| Heliocentric radial velocity | 2,216 km/s |
| Distance | 109 Mly (33.4 Mpc) |
| Apparent magnitude (V) | 15.7 |
| Other designations | |
| PGC 61361, UGC 11105, MCG +04-42-024, Z 141-47 | |
UGC 11105 known as PGC 61361, is a relatively nearby spiral galaxy located 109 million light-years away in the Hercules constellation. [1] It is less luminous in appearance. The supernova that occurred in UGC 11105 in 2019, has long faded. [2] It is outshone by the bright stars shown in the foreground. [2] From the perspective on Earth, the Sun is 14 thousand trillion times brighter as compared to UGC 1105, if we to calculate the apparent magnitude for both objects. [2] It is a possible active galactic nucleus candidate, according to SIMBAD. [3]
References
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-20.
- ^ a b c information@eso.org. "Dim, but still distinct". www.spacetelescope.org. Retrieved 2024-04-20.
- ^ "UGC 11105". simbad.u-strasbg.fr. Retrieved 2024-04-20.
| UGC 11105 | |
|---|---|
|
Hubble Space Telescope image of UGC 11105 | |
| Observation data | |
| Constellation | Hercules |
| Right ascension | 271.1 degrees |
| Redshift | 0.007418 0.000013 |
| Heliocentric radial velocity | 2,216 km/s |
| Distance | 109 Mly (33.4 Mpc) |
| Apparent magnitude (V) | 15.7 |
| Other designations | |
| PGC 61361, UGC 11105, MCG +04-42-024, Z 141-47 | |
UGC 11105 known as PGC 61361, is a relatively nearby spiral galaxy located 109 million light-years away in the Hercules constellation. [1] It is less luminous in appearance. The supernova that occurred in UGC 11105 in 2019, has long faded. [2] It is outshone by the bright stars shown in the foreground. [2] From the perspective on Earth, the Sun is 14 thousand trillion times brighter as compared to UGC 1105, if we to calculate the apparent magnitude for both objects. [2] It is a possible active galactic nucleus candidate, according to SIMBAD. [3]
References
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-20.
- ^ a b c information@eso.org. "Dim, but still distinct". www.spacetelescope.org. Retrieved 2024-04-20.
- ^ "UGC 11105". simbad.u-strasbg.fr. Retrieved 2024-04-20.