IC 1296
| IC 1296 | |
|---|---|
 IC 1296, as seen by Spitzer | |
| Observation data (J2000 epoch) | |
| Constellation | Lyra |
| Right ascension | 18h 53m 18s |
| Declination | +33° 03’ 59” |
| Redshift | 0.017075 |
| Heliocentric radial velocity | 5,119 km/s |
| Distance | 238 Mly (72.97 Mpc) |
| Surface brightness | 23.63 mag/arcsec^2 |
| Characteristics | |
| Type | SBbc |
| Size | 120,000 ly |
| Apparent size (V) | 1.10' x 0.9' |
| Other designations | |
| IC 1296, UGC 11374, PGC 62532, CGCG 201-040, MCG +06-41-022, 2MASX J18531883+3303596, 2MASS J18531884+3303599 | |
IC 1296 is an extremely faint barred spiral galaxy of Hubble-type SBbc in the constellation Lyra in the northern sky. It is estimated to be 238 million light-years from the Milky Way and about 120,000 light-years in diameter.[1]
IC 1296 is only 4 arc minutes away from the well-known Ring Nebula in the night sky.[2] Planetary nebulae and galaxies are rarely observed together because planetary nebulae are galactic objects and are concentrated toward our galactic center, where extragalactic objects - such as distant galaxies - are rarely observed due to absorption by gas and dust.
The astronomical object was discovered on October 2, 1893, by Edward Emerson Barnard. In August 2013, supernova SN2013ev[3] was discovered in the southern spiral arm of IC 1296.[4]
See also
[edit]External links
[edit]References
[edit]- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-06-06.
- ^ "Ring Nebula (Messier 57) | Deep⋆Sky Corner". www.deepskycorner.ch. Retrieved 2024-06-06.
- ^ "IC 1296", Wikipedia (in German), 2024-04-29, retrieved 2024-06-06
- ^ "Revised IC Data for IC 1296". spider.seds.org. Retrieved 2024-06-06.