Star · A0V
HIP 26862
HIP 26862 is a main-sequence star of spectral type A0V in the constellation Columba, 635.5 light-years from the Sun.
| Constellation | Columba |
|---|---|
| Distance | 635.5 light-years (194.8 pc) |
| Apparent magnitude | magnitude 6.18 |
| Absolute magnitude | magnitude −0.27 |
| Spectral type | A0V |
| Surface temperature | 9,850 K |
| Luminosity | 147 L☉ |
| Radius | 4.17 R☉ |
| Mass | 3.78 M☉ (estimated) |
| Right ascension (J2000) | 5h 42m 11.6s |
| Declination (J2000) | −30° 32′ 08″ |
| Space velocity (relative to the Sun) | 27.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.18). Visible from the whole Southern Hemisphere and north to latitude 59° N. South of latitude 59° 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 1391. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 11 million years.
The Sun seen from there
From a planet around HIP 26862, the Sun would look like a star of magnitude 11.28, 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.