Star · G5V
GJ 4050
GJ 4050 is a main-sequence star of spectral type G5V in the constellation Telescopium, 156.9 light-years from the Sun.
| Other names | HIP 89855 |
|---|---|
| Constellation | Telescopium |
| Distance | 156.9 light-years (48.1 pc) |
| Apparent magnitude | magnitude 7.34 |
| Absolute magnitude | magnitude 3.93 |
| Spectral type | G5V |
| Surface temperature | 5,410 K |
| Luminosity | 2.72 L☉ |
| Radius | 1.88 R☉ |
| Mass | 1.28 M☉ (estimated) |
| Right ascension (J2000) | 18h 20m 11.5s |
| Declination (J2000) | −45° 55′ 20″ |
| Space velocity (relative to the Sun) | 43.1 km/s |
In the sky
Too faint for the naked eye (magnitude 7.34); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 44° N. South of latitude 44° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1869. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.8 million years.
The Sun seen from there
From a planet around GJ 4050, the Sun would look like a star of magnitude 8.24, in the direction where our sky has the constellation Auriga. 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.