Star · G2V
Gl 392B
Gl 392B is a main-sequence star of spectral type G2V in the constellation Ursa Major, 75.0 light-years from the Sun.
| Constellation | Ursa Major |
|---|---|
| Distance | 75.0 light-years (23.0 pc) |
| Apparent magnitude | magnitude 12.50 |
| Absolute magnitude | magnitude 10.69 |
| Spectral type | G2V |
| Surface temperature | 5,780 K |
| Luminosity | 0.00491 L☉ |
| Radius | 0.0699 R☉ |
| Mass | 0.188 M☉ (estimated) |
| Right ascension (J2000) | 10h 28m 03.9s |
| Declination (J2000) | +48° 47′ 11″ |
| Space velocity (relative to the Sun) | 98.1 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.50. Visible from the whole Northern Hemisphere and south to latitude 41° S. North of latitude 41° N it never sets. It stands highest at midnight in February, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1951. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.3 million years.
The Sun seen from there
From a planet around Gl 392B, the Sun would look like a star of magnitude 6.64, in the direction where our sky has the constellation Grus. It would be invisible 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.