| NGC 2927 | |
|---|---|
 NGC 2927 imaged bySDSS | |
| Observation data (J2000epoch) | |
| Constellation | Leo |
| Right ascension | 09h 37m 15.2100s[1] |
| Declination | +23° 35′ 26.209″[1] |
| Redshift | 0.025147[1] |
| Heliocentric radial velocity | 7539 ± 2 km/s[1] |
| Distance | 393.56 ± 2.88 Mly (120.667 ± 0.882 Mpc)[1] |
| Apparent magnitude (V) | 12.9[1] |
| Characteristics | |
| Type | SAB(rs)b[1] |
| Size | ~229,000 ly (70.20 kpc) (estimated)[1] |
| Apparent size (V) | 1.3′ × 1.0′[1] |
| Other designations | |
| IRAS F09343+2349,2MASX J09371521+2335261,UGC 5122,MCG +04-23-016,PGC 27385,CGCG 122-032[1] | |
NGC 2927 is a largebarred spiral galaxy in theconstellation ofLeo. Its velocity with respect to thecosmic microwave background is 7830 ± 20 km/s, which corresponds to aHubble distance of 376.7 ± 26.4 Mly (115.49 ± 8.09 Mpc).[1] In addition, threenon-redshift measurements give a distance of 393.56 ± 2.88 Mly (120.667 ± 0.882 Mpc).[2] The galaxy was discovered by German astronomerHeinrich d'Arrest on 21 February 1863.[3]
TheSIMBAD database lists NGC 2927 as aradio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure.[4]
Onesupernova has been observed in NGC 2927: SN 2023uvg (Type Ic, mag. 18.7389) was discovered by theAutomatic Learning for the Rapid Classification of Events (ALeRCE) on 13 October 2023.[5]
NGC 2927 forms apair of galaxies withNGC 2929.[6]
Media related toNGC 2927 at Wikimedia Commons
