Star · M4III
HIP 106062
HIP 106062 is a giant star of spectral type M4III in the constellation Pegasus, 833.7 light-years from the Sun.
| Constellation | Pegasus |
|---|---|
| Distance | 833.7 light-years (255.6 pc) |
| Apparent magnitude | magnitude 5.84 |
| Absolute magnitude | magnitude −1.20 |
| Spectral type | M4III |
| Surface temperature | 4,000 K |
| Luminosity | 738 L☉ |
| Radius | 56.6 R☉ |
| Mass | 5.99 M☉ (estimated) |
| Right ascension (J2000) | 21h 28m 59.8s |
| Declination (J2000) | +22° 10′ 46″ |
| Space velocity (relative to the Sun) | 50.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.84). Visible from the whole Northern Hemisphere and south to latitude 68° S. North of latitude 68° N it never sets. It stands highest at midnight in August, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1192. 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 106062, the Sun would look like a star of magnitude 11.87, in the direction where our sky has the constellation Hydra. 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.