Star · K5III
HIP 38206
HIP 38206 is a giant star of spectral type K5III in the constellation Puppis, 1,478 light-years from the Sun.
| Constellation | Puppis |
|---|---|
| Distance | 1,478 light-years (453.1 pc) |
| Apparent magnitude | magnitude 6.34 |
| Absolute magnitude | magnitude −1.94 |
| Spectral type | K5III |
| Surface temperature | 3,570 K |
| Luminosity | 2,620 L☉ |
| Radius | 134 R☉ |
| Mass | 8.61 M☉ (estimated) |
| Right ascension (J2000) | 7h 49m 40.0s |
| Declination (J2000) | −14° 05′ 07″ |
| Space velocity (relative to the Sun) | 36.6 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.34). Visible from the whole Southern Hemisphere and north to latitude 76° N. South of latitude 76° S it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 548. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 26 million years.
The Sun seen from there
From a planet around HIP 38206, the Sun would look like a star of magnitude 13.11, in the direction where our sky has the constellation Aquila. 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.