Star · B2V
HIP 39530
HIP 39530 is a main-sequence star of spectral type B2V in the constellation Carina, 1,375 light-years from the Sun.
| Constellation | Carina |
|---|---|
| Distance | 1,375 light-years (421.7 pc) |
| Apparent magnitude | magnitude 6.25 |
| Absolute magnitude | magnitude −1.87 |
| Spectral type | B2V |
| Surface temperature | 11,460 K |
| Luminosity | 839 L☉ |
| Radius | 7.35 R☉ |
| Mass | 6.22 M☉ (estimated) |
| Right ascension (J2000) | 8h 04m 42.9s |
| Declination (J2000) | −62° 50′ 11″ |
| Space velocity (relative to the Sun) | 26.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.25). Visible from the whole Southern Hemisphere and north to latitude 27° N. South of latitude 27° S it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 651. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 24 million years.
The Sun seen from there
From a planet around HIP 39530, the Sun would look like a star of magnitude 12.95, in the direction where our sky has the constellation Draco. 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.