Star · B9V
HIP 115759
HIP 115759 is a main-sequence star of spectral type B9V in the constellation Phoenix, 478.0 light-years from the Sun.
| Constellation | Phoenix |
|---|---|
| Distance | 478.0 light-years (146.5 pc) |
| Apparent magnitude | magnitude 6.22 |
| Absolute magnitude | magnitude 0.39 |
| Spectral type | B9V |
| Surface temperature | 11,250 K |
| Luminosity | 101 L☉ |
| Radius | 2.64 R☉ |
| Mass | 3.39 M☉ (estimated) |
| Right ascension (J2000) | 23h 27m 09.1s |
| Declination (J2000) | −50° 09′ 26″ |
| Space velocity (relative to the Sun) | 21.9 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.22). Visible from the whole Southern Hemisphere and north to latitude 40° N. South of latitude 40° S it never sets. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1548. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 8.5 million years.
The Sun seen from there
From a planet around HIP 115759, the Sun would look like a star of magnitude 10.66, in the direction where our sky has the constellation Ursa Major. 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.