Star · K0
HIP 38307
HIP 38307 is a supergiant star of spectral type K0 in the constellation Monoceros, 435.0 light-years from the Sun.
| Constellation | Monoceros |
|---|---|
| Distance | 435.0 light-years (133.4 pc) |
| Apparent magnitude | magnitude 6.16 |
| Absolute magnitude | magnitude 0.53 |
| Spectral type | K0 |
| Surface temperature | 4,460 K |
| Luminosity | 98.7 L☉ |
| Radius | 16.7 R☉ |
| Mass | 3.37 M☉ (estimated) |
| Right ascension (J2000) | 7h 50m 55.2s |
| Declination (J2000) | −11° 07′ 43″ |
| Space velocity (relative to the Sun) | 51.1 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.16). Visible from the whole Southern Hemisphere and north to latitude 79° N. South of latitude 79° 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 1591. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 7.7 million years.
The Sun seen from there
From a planet around HIP 38307, the Sun would look like a star of magnitude 10.46, 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.