Star · B8V
HIP 93887
HIP 93887 is a main-sequence star of spectral type B8V in the constellation Sagittarius, 700.7 light-years from the Sun.
| Constellation | Sagittarius |
|---|---|
| Distance | 700.7 light-years (214.8 pc) |
| Apparent magnitude | magnitude 6.28 |
| Absolute magnitude | magnitude −0.38 |
| Spectral type | B8V |
| Surface temperature | 10,710 K |
| Luminosity | 187 L☉ |
| Radius | 3.98 R☉ |
| Mass | 4.05 M☉ (estimated) |
| Right ascension (J2000) | 19h 07m 08.3s |
| Declination (J2000) | −18° 44′ 17″ |
| Space velocity (relative to the Sun) | 25.7 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.28). Visible from the whole Southern Hemisphere and north to latitude 71° N. South of latitude 71° S it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1325. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 12 million years.
The Sun seen from there
From a planet around HIP 93887, the Sun would look like a star of magnitude 11.49, in the direction where our sky has the constellation Gemini. 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.