Star · G6
HIP 101427
HIP 101427 is a supergiant star of spectral type G6 in the constellation Octans, 761.6 light-years from the Sun.
| Constellation | Octans |
|---|---|
| Distance | 761.6 light-years (233.5 pc) |
| Apparent magnitude | magnitude 5.76 |
| Absolute magnitude | magnitude −1.08 |
| Spectral type | G6 |
| Surface temperature | 4,470 K |
| Luminosity | 434 L☉ |
| Radius | 34.8 R☉ |
| Mass | 5.15 M☉ (estimated) |
| Right ascension (J2000) | 20h 33m 17.7s |
| Declination (J2000) | −80° 57′ 54″ |
| Space velocity (relative to the Sun) | 21.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.76). Visible from the whole Southern Hemisphere and north to latitude 9° N. South of latitude 9° S it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1264. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 14 million years.
The Sun seen from there
From a planet around HIP 101427, the Sun would look like a star of magnitude 11.67, in the direction where our sky has the constellation Camelopardalis. 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.