Star · B9IV
HIP 92394
HIP 92394 is a subgiant star of spectral type B9IV in the constellation Pavo, 866.6 light-years from the Sun.
| Constellation | Pavo |
|---|---|
| Distance | 866.6 light-years (265.7 pc) |
| Apparent magnitude | magnitude 6.04 |
| Absolute magnitude | magnitude −1.08 |
| Spectral type | B9IV |
| Surface temperature | 9,730 K |
| Luminosity | 306 L☉ |
| Radius | 6.16 R☉ |
| Mass | 4.66 M☉ (estimated) |
| Right ascension (J2000) | 18h 49m 43.7s |
| Declination (J2000) | −72° 59′ 45″ |
| Space velocity (relative to the Sun) | 19.0 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.04). Visible from the whole Southern Hemisphere and north to latitude 17° N. South of latitude 17° 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 1159. 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 92394, the Sun would look like a star of magnitude 11.95, in the direction where our sky has the constellation Camelopardalis. 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.