Star · K3V
Gl 4.2B
Gl 4.2B is a main-sequence star of spectral type K3V in the constellation Phoenix, 85.3 light-years from the Sun.
| Constellation | Phoenix |
|---|---|
| Distance | 85.3 light-years (26.2 pc) |
| Apparent magnitude | magnitude 11.50 |
| Absolute magnitude | magnitude 9.41 |
| Spectral type | K3V |
| Surface temperature | 4,670 K |
| Luminosity | 0.024 L☉ |
| Radius | 0.237 R☉ |
| Mass | 0.374 M☉ (estimated) |
| Right ascension (J2000) | 0h 06m 17.7s |
| Declination (J2000) | −49° 04′ 35″ |
| Space velocity (relative to the Sun) | 70.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.50. Visible from the whole Southern Hemisphere and north to latitude 41° N. South of latitude 41° S it never sets. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1941. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.5 million years.
The Sun seen from there
From a planet around Gl 4.2B, the Sun would look like a star of magnitude 6.92, in the direction where our sky has the constellation Ursa Major. 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.