NGC 3535 is a spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 7289 ± 25 km/s, which corresponds to a Hubble distance of 107.51 ± 7.54 Mpc (∼351 million light-years).[1] It was discovered by German-British astronomer William Herschel on 18 April 1784.
| NGC 3535 | |
|---|---|
 The spiral galaxy NGC 3535. | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 08m 33.92s[1] |
| Declination | +04° 49′ 54.821″[1] |
| Redshift | 0.023103[1] |
| Heliocentric radial velocity | 6926 ± 2 km/s[1] |
| Distance | 350.7 ± 24.6 Mly (107.51 ± 7.54 Mpc)[1] |
| Apparent magnitude (V) | 13.5[1] |
| Characteristics | |
| Type | SA(s)a pec?[1] |
| Size | ~162,300 ly (49.77 kpc) (estimated)[1] |
| Apparent size (V) | 1.7' x 0.8'[1] |
| Other designations | |
| IRAS 11059+0505, 2MASX J11083390+0449545, UGC 6189, MCG +01-29-004, PGC 33760, CGCG 039-010[1] | |
According to the SIMBAD database, NGC 3535 is a radio galaxy.[2]
One supernova has been observed in NGC 3535: SN 2023hrn (type Ia, mag. 18.4).[3]
See also
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Media related to NGC 3535 at Wikimedia Commons- NGC 3535 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
