Star · B9V
14 CVn
14 CVn is a main-sequence star of spectral type B9V in the constellation Canes Venatici, 331.6 light-years from the Sun.
| Other names | HIP 63901 |
|---|---|
| Constellation | Canes Venatici |
| Distance | 331.6 light-years (101.7 pc) |
| Apparent magnitude | magnitude 5.20 |
| Absolute magnitude | magnitude 0.16 |
| Spectral type | B9V |
| Surface temperature | 10,930 K |
| Luminosity | 118 L☉ |
| Radius | 3.03 R☉ |
| Mass | 3.55 M☉ (estimated) |
| Right ascension (J2000) | 13h 05m 44.4s |
| Declination (J2000) | +35° 47′ 56″ |
| Space velocity (relative to the Sun) | 25.1 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.20). Visible from the whole Northern Hemisphere and south to latitude 54° S. North of latitude 54° N it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1694. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.9 million years.
The Sun seen from there
From a planet around 14 CVn, the Sun would look like a star of magnitude 9.87, in the direction where our sky has the constellation Sculptor. It would be invisible to the naked eye.
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.