Star · B5V
HIP 91119
HIP 91119 is a main-sequence star of spectral type B5V in the constellation Lyra, 817.4 light-years from the Sun.
| Constellation | Lyra |
|---|---|
| Distance | 817.4 light-years (250.6 pc) |
| Apparent magnitude | magnitude 6.10 |
| Absolute magnitude | magnitude −0.90 |
| Spectral type | B5V |
| Surface temperature | 11,830 K |
| Luminosity | 362 L☉ |
| Radius | 4.53 R☉ |
| Mass | 4.89 M☉ (estimated) |
| Right ascension (J2000) | 18h 35m 13.5s |
| Declination (J2000) | +34° 27′ 29″ |
| Space velocity (relative to the Sun) | 27.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.10). Visible from the whole Northern Hemisphere and south to latitude 56° S. North of latitude 56° N 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 1209. 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 91119, the Sun would look like a star of magnitude 11.83, in the direction where our sky has the constellation Columba. 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.