Star · B3V
HIP 93177
HIP 93177 is a main-sequence star of spectral type B3V in the constellation Lyra, 1,122 light-years from the Sun.
| Constellation | Lyra |
|---|---|
| Distance | 1,122 light-years (344.1 pc) |
| Apparent magnitude | magnitude 6.20 |
| Absolute magnitude | magnitude −1.48 |
| Spectral type | B3V |
| Surface temperature | 12,410 K |
| Luminosity | 685 L☉ |
| Radius | 5.66 R☉ |
| Mass | 5.87 M☉ (estimated) |
| Right ascension (J2000) | 18h 58m 46.6s |
| Declination (J2000) | +40° 40′ 45″ |
| Space velocity (relative to the Sun) | 14.4 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.20). Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N 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 904. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 20 million years.
The Sun seen from there
From a planet around HIP 93177, the Sun would look like a star of magnitude 12.51, in the direction where our sky has the constellation Puppis. 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.