Star · K3V
Gl 612
Gl 612 is a main-sequence star of spectral type K3V in the constellation Corona Borealis, 75.8 light-years from the Sun.
| Other names | HIP 78913 |
|---|---|
| Constellation | Corona Borealis |
| Distance | 75.8 light-years (23.2 pc) |
| Apparent magnitude | magnitude 8.58 |
| Absolute magnitude | magnitude 6.75 |
| Spectral type | K3V |
| Surface temperature | 4,830 K |
| Luminosity | 0.255 L☉ |
| Radius | 0.72 R☉ |
| Mass | 0.71 M☉ (estimated) |
| Right ascension (J2000) | 16h 06m 29.6s |
| Declination (J2000) | +38° 37′ 56″ |
| Space velocity (relative to the Sun) | 68.5 km/s |
In the sky
Too faint for the naked eye (magnitude 8.58); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 51° S. North of latitude 51° N it never sets. 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 1950. 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 612, the Sun would look like a star of magnitude 6.66, in the direction where our sky has the constellation Eridanus. 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.