Star · M0III
HIP 93770
HIP 93770 is a giant star of spectral type M0III in the constellation Lyra, 1,175 light-years from the Sun.
| Constellation | Lyra |
|---|---|
| Distance | 1,175 light-years (360.2 pc) |
| Apparent magnitude | magnitude 6.32 |
| Absolute magnitude | magnitude −1.46 |
| Spectral type | M0III |
| Surface temperature | 3,560 K |
| Luminosity | 1,720 L☉ |
| Radius | 109 R☉ |
| Mass | 7.63 M☉ (estimated) |
| Right ascension (J2000) | 19h 05m 47.1s |
| Declination (J2000) | +29° 55′ 18″ |
| Space velocity (relative to the Sun) | 32.4 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.32). Visible from the whole Northern Hemisphere and south to latitude 60° S. North of latitude 60° 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 851. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 21 million years.
The Sun seen from there
From a planet around HIP 93770, the Sun would look like a star of magnitude 12.61, in the direction where our sky has the constellation Canis Major. 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.