19 Canum Venaticorum
From Wikipedia, the free encyclopedia
| Observation data Equinox J2000.0 |
|
|---|---|
| Constellation | Canes Venatici |
| Right ascension | 13h15m32.0s |
| Declination | +40°51′19″ |
| Apparent magnitude (V) | +5.77 |
| Distance | 245 ± 14 ly (75 ± 4 pc) |
| Spectral type | A7V |
| Other designations | |
19 Canum Venaticorum is a binary star in the constellation Canes Venatici. It is approximately 245 light years from Earth.
The primary component, 19 Canum Venaticorum A, is a white A-type main sequence dwarf with an apparent magnitude of +5.77. It's companion, 19 Canum Venaticorum B, is a tenth magnitude star located only 0.37 arcseconds from the primary.
 |
This binary or multiple star system–related article is a stub. You can help Wikipedia by expanding it. |
