Star · M2
Gl 250B
Gl 250B is a main-sequence star of spectral type M2 in the constellation Monoceros, 28.5 light-years from the Sun.
| Constellation | Monoceros |
|---|---|
| Distance | 28.5 light-years (8.75 pc) |
| Apparent magnitude | magnitude 10.09 |
| Absolute magnitude | magnitude 10.38 |
| Spectral type | M2 |
| Surface temperature | 3,790 K |
| Luminosity | 0.0222 L☉ |
| Radius | 0.345 R☉ |
| Mass | 0.362 M☉ (estimated) |
| Right ascension (J2000) | 6h 52m 18.4s |
| Declination (J2000) | −5° 11′ 24″ |
| Space velocity (relative to the Sun) | 25.1 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 10.09. Visible from the whole Southern Hemisphere and north to latitude 85° N. 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 1997. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 506 thousand years.
The Sun seen from there
From a planet around Gl 250B, the Sun would look like a star of magnitude 4.54, in the direction where our sky has the constellation Serpens. 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.