Star · K0V
Gl 264.1B
Gl 264.1B is a main-sequence star of spectral type K0V in the constellation Puppis, 55.6 light-years from the Sun.
| Other names | HIP 34069 |
|---|---|
| Constellation | Puppis |
| Distance | 55.6 light-years (17.1 pc) |
| Apparent magnitude | magnitude 6.83 |
| Absolute magnitude | magnitude 5.67 |
| Spectral type | K0V |
| Surface temperature | 5,340 K |
| Luminosity | 0.557 L☉ |
| Radius | 0.871 R☉ |
| Mass | 0.864 M☉ (estimated) |
| Right ascension (J2000) | 7h 03m 58.9s |
| Declination (J2000) | −43° 36′ 40″ |
| Space velocity (relative to the Sun) | 94.2 km/s |
In the sky
Too faint for the naked eye (magnitude 6.83); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 46° N. South of latitude 46° 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 1970. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 987 thousand years.
The Sun seen from there
From a planet around Gl 264.1B, the Sun would look like a star of magnitude 5.99, in the direction where our sky has the constellation Lyra. It would be visible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.