Star · M4
GJ 3937
GJ 3937 is a main-sequence star of spectral type M4 in the constellation Ophiuchus, 57.2 light-years from the Sun.
| Constellation | Ophiuchus |
|---|---|
| Distance | 57.2 light-years (17.5 pc) |
| Apparent magnitude | magnitude 15.51 |
| Absolute magnitude | magnitude 14.29 |
| Spectral type | M4 |
| Surface temperature | 3,290 K |
| Luminosity | 0.00142 L☉ |
| Radius | 0.116 R☉ |
| Mass | 0.109 M☉ (estimated) |
| Right ascension (J2000) | 16h 04m 19.7s |
| Declination (J2000) | −6° 16′ 51″ |
| Space velocity (relative to the Sun) | 72.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 15.51. Visible from the whole Southern Hemisphere and north to latitude 84° N. It stands highest at midnight in May, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1969. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.0 million years.
The Sun seen from there
From a planet around GJ 3937, the Sun would look like a star of magnitude 6.05, in the direction where our sky has the constellation Taurus. 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.