Star · B5V
HIP 69491
HIP 69491 is a main-sequence star of spectral type B5V in the constellation Centaurus, 827.3 light-years from the Sun.
| Constellation | Centaurus |
|---|---|
| Distance | 827.3 light-years (253.6 pc) |
| Apparent magnitude | magnitude 6.09 |
| Absolute magnitude | magnitude −0.93 |
| Spectral type | B5V |
| Surface temperature | 9,530 K |
| Luminosity | 259 L☉ |
| Radius | 5.9 R☉ |
| Mass | 4.44 M☉ (estimated) |
| Right ascension (J2000) | 14h 13m 39.8s |
| Declination (J2000) | −54° 37′ 32″ |
| Space velocity (relative to the Sun) | 71.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.09). Visible from the whole Southern Hemisphere and north to latitude 35° N. South of latitude 35° S 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 1199. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 15 million years.
The Sun seen from there
From a planet around HIP 69491, the Sun would look like a star of magnitude 11.85, in the direction where our sky has the constellation Perseus. 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.