| NGC 3535 | |
|---|---|
 NGC 3535 imaged byLegacy Surveys | |
| Observation data (J2000epoch) | |
| Constellation | Leo |
| Right ascension | 11h 08m 33.9105s[1] |
| Declination | +04° 49′ 54.781″[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′ × 0.8′[1] |
| Other designations | |
| IRAS 11059+0505,2MASX J11083390+0449545,UGC 6189,MCG +01-29-004,PGC 33760,CGCG 039-010[1] | |
NGC 3535 is an unbarredspiral galaxy in theconstellation ofLeo. Its velocity with respect to thecosmic microwave background is7,289±25 km/s, which corresponds to aHubble distance of 350.7 ± 24.6 Mly (107.51 ± 7.54 Mpc).[1] It was discovered by German-British astronomerWilliam Herschel on 18 April 1784.[2][3]
According to theSIMBAD database, NGC 3535 is aradio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure.[4]
Onesupernova has been observed in NGC 3535:SN 2023hrn (Type Ia, mag. 18.4) was discovered byATLAS on 8 May 2023.[5]
Media related toNGC 3535 at Wikimedia Commons
