Star · B3V
16 Peg
16 Peg is a main-sequence star of spectral type B3V in the constellation Pegasus, 561.4 light-years from the Sun.
| Other names | HIP 108022 |
|---|---|
| Constellation | Pegasus |
| Distance | 561.4 light-years (172.1 pc) |
| Apparent magnitude | magnitude 5.09 |
| Absolute magnitude | magnitude −1.09 |
| Spectral type | B3V |
| Surface temperature | 12,590 K |
| Luminosity | 490 L☉ |
| Radius | 4.65 R☉ |
| Mass | 5.33 M☉ (estimated) |
| Right ascension (J2000) | 21h 53m 03.8s |
| Declination (J2000) | +25° 55′ 31″ |
| Space velocity (relative to the Sun) | 14.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.09). Visible from the whole Northern Hemisphere and south to latitude 64° S. North of latitude 64° 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 1465. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 10.0 million years.
The Sun seen from there
From a planet around 16 Peg, the Sun would look like a star of magnitude 11.01, 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.