Star · B9V
HIP 26796
HIP 26796 is a main-sequence star of spectral type B9V in the constellation Columba, 409.3 light-years from the Sun.
| Constellation | Columba |
|---|---|
| Distance | 409.3 light-years (125.5 pc) |
| Apparent magnitude | magnitude 6.35 |
| Absolute magnitude | magnitude 0.86 |
| Spectral type | B9V |
| Surface temperature | 10,650 K |
| Luminosity | 59.4 L☉ |
| Radius | 2.26 R☉ |
| Mass | 2.92 M☉ (estimated) |
| Right ascension (J2000) | 5h 41m 26.9s |
| Declination (J2000) | −33° 24′ 03″ |
| Space velocity (relative to the Sun) | 34.8 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.35). Visible from the whole Southern Hemisphere and north to latitude 57° N. South of latitude 57° S it never sets. It stands highest at midnight in December, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1617. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.3 million years.
The Sun seen from there
From a planet around HIP 26796, the Sun would look like a star of magnitude 10.32, in the direction where our sky has the constellation Hercules. 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.