Star · B6I
HIP 87460
HIP 87460 is a supergiant star of spectral type B6I in the constellation Scorpius, 904.4 light-years from the Sun.
| Constellation | Scorpius |
|---|---|
| Distance | 904.4 light-years (277.3 pc) |
| Apparent magnitude | magnitude 5.88 |
| Absolute magnitude | magnitude −1.33 |
| Spectral type | B6I |
| Surface temperature | 11,760 K |
| Luminosity | 536 L☉ |
| Radius | 5.58 R☉ |
| Mass | 5.47 M☉ (estimated) |
| Right ascension (J2000) | 17h 52m 13.7s |
| Declination (J2000) | −34° 47′ 57″ |
| Space velocity (relative to the Sun) | 15.7 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.88). Visible from the whole Southern Hemisphere and north to latitude 55° N. South of latitude 55° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1122. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 16 million years.
The Sun seen from there
From a planet around HIP 87460, the Sun would look like a star of magnitude 12.04, in the direction where our sky has the constellation Auriga. 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.