IC 3786
| IC 3786 | |
|---|---|
 Sloan Digital Sky Survey image of IC 3786 | |
| Observation data | |
| Constellation | Canes Venatici |
| Right ascension | 191.90 degrees |
| Declination | 39.04 degrees |
| Redshift | 0.05472 0.00002 |
| Heliocentric radial velocity | 16,036 km/s |
| Distance | 755 Mly (231.5 Mpc) |
| Apparent magnitude (V) | 20.16 |
| Surface brightness | 22.9 mag/arcsec |
| Characteristics | |
| Type | Sbc |
| Other designations | |
| PGC 2142309, 2MASX J12473689+3902461, ASK 507092.0, NPM1G +39.0301, SDSS J124736.89+390245.6, NSA 088286, 2MASS J12473689+3902461, LEDA 2142309 | |
IC 3786 is a type Sbc[1] spiral galaxy in the Canes Venatici constellation.[2][3] It is located 755 million light-years[4] from the Milky Way and was discovered by Max Wolf on March 21, 1903.[5]
References
- ^ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-04-26.
- ^ "Revised IC Data for IC 3786". spider.seds.org. Retrieved 2024-04-26.
- ^ Astronomy, Go. "IC 3786 | galaxy in Canes Venatici | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-04-26.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-26.
- ^ "Index Catalog Objects: IC 3750 - 3799". cseligman.com. Retrieved 2024-04-26.
