Star · B3V
HIP 75959
HIP 75959 is a main-sequence star of spectral type B3V in the constellation Apus, 1,096 light-years from the Sun.
| Constellation | Apus |
|---|---|
| Distance | 1,096 light-years (336.0 pc) |
| Apparent magnitude | magnitude 6.39 |
| Absolute magnitude | magnitude −1.24 |
| Spectral type | B3V |
| Surface temperature | 11,780 K |
| Luminosity | 494 L☉ |
| Radius | 5.34 R☉ |
| Mass | 5.34 M☉ (estimated) |
| Right ascension (J2000) | 15h 30m 49.2s |
| Declination (J2000) | −71° 39′ 15″ |
| Space velocity (relative to the Sun) | 35.1 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.39). Visible from the whole Southern Hemisphere and north to latitude 18° N. South of latitude 18° S it never sets. It stands highest at midnight in May, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 930. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 19 million years.
The Sun seen from there
From a planet around HIP 75959, the Sun would look like a star of magnitude 12.46, in the direction where our sky has the constellation Cassiopeia. 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.