Star · M2
Gl 767B
Gl 767B is a main-sequence star of spectral type M2 in the constellation Cygnus, 45.5 light-years from the Sun.
| Constellation | Cygnus |
|---|---|
| Distance | 45.5 light-years (14.0 pc) |
| Apparent magnitude | magnitude 11.10 |
| Absolute magnitude | magnitude 10.38 |
| Spectral type | M2 |
| Surface temperature | 3,760 K |
| Luminosity | 0.0231 L☉ |
| Radius | 0.358 R☉ |
| Mass | 0.368 M☉ (estimated) |
| Right ascension (J2000) | 19h 46m 23.9s |
| Declination (J2000) | +32° 01′ 02″ |
| Space velocity (relative to the Sun) | 42.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.10. Visible from the whole Northern Hemisphere and south to latitude 58° S. North of latitude 58° N it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1981. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 807 thousand years.
The Sun seen from there
From a planet around Gl 767B, the Sun would look like a star of magnitude 5.55, in the direction where our sky has the constellation Puppis. 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.