Star · K4V
Gl 485
Gl 485 is a main-sequence star of spectral type K4V in the constellation Coma Berenices, 94.3 light-years from the Sun.
| Other names | HIP 62406 |
|---|---|
| Constellation | Coma Berenices |
| Distance | 94.3 light-years (28.9 pc) |
| Apparent magnitude | magnitude 9.86 |
| Absolute magnitude | magnitude 7.56 |
| Spectral type | K4V |
| Surface temperature | 4,170 K |
| Luminosity | 0.196 L☉ |
| Radius | 0.848 R☉ |
| Mass | 0.665 M☉ (estimated) |
| Right ascension (J2000) | 12h 47m 20.1s |
| Declination (J2000) | +31° 12′ 49″ |
| Space velocity (relative to the Sun) | 33.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.86. Visible from the whole Northern Hemisphere and south to latitude 59° S. North of latitude 59° N it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1932. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.7 million years.
The Sun seen from there
From a planet around Gl 485, the Sun would look like a star of magnitude 7.13, in the direction where our sky has the constellation Sculptor. 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.