Star · M0III
HIP 94630
HIP 94630 is a giant star of spectral type M0III in the constellation Lyra, 953.5 light-years from the Sun.
| Constellation | Lyra |
|---|---|
| Distance | 953.5 light-years (292.3 pc) |
| Apparent magnitude | magnitude 5.88 |
| Absolute magnitude | magnitude −1.45 |
| Spectral type | M0III |
| Surface temperature | 3,560 K |
| Luminosity | 1,690 L☉ |
| Radius | 108 R☉ |
| Mass | 7.59 M☉ (estimated) |
| Right ascension (J2000) | 19h 15m 24.9s |
| Declination (J2000) | +30° 31′ 35″ |
| Space velocity (relative to the Sun) | 87.9 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.88). Visible from the whole Northern Hemisphere and south to latitude 59° S. North of latitude 59° 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 1072. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 17 million years.
The Sun seen from there
From a planet around HIP 94630, the Sun would look like a star of magnitude 12.16, 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.