NGC 3753
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| NGC 3753 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 37m 53.90s |
| Declination | +21d 58m 53.0s |
| Redshift | 0.029064 |
| Heliocentric radial velocity | 8,713 km/s |
| Distance | 435 Mly (133.37 Mpc) |
| Group or cluster | Copeland Septet |
| Apparent magnitude (V) | 14.52 |
| Characteristics | |
| Type | Sb, LINER, SAb |
| Size | 258,000 ly |
| Other designations | |
| PGC 36016, UGC 6602, VV 282a, KUG 1135+222, MCG +04-28-010, SPRC 203, Copeland Septet NED06, HCG 057A, 2MASS J11375380+2158520, 2MASX J11375378+2158520, SDSS J113753.78+215851.8, WBL 343-005, NSA 139944, SSTL2 J113753.80+215852.4, LEDA 36016 | |
NGC 3753 is a large barred spiral galaxy located in the Leo constellation.[1] It is located 435 million light-years away from the earth[2] and was discovered on February 9, 1874, by Ralph Copeland.[3]
NGC 3753 is classified as a LINER galaxy, meaning it presents an emission spectrum characterized by broad lines of weak ionized atoms. It also has a luminosity class of I-II.[2] NGC 3753 is viewed edge-on. The edge-on view is the reason why we see a dust lane in NGC 3753.
