Star · K0
HIP 79385
HIP 79385 is a supergiant star of spectral type K0 in the constellation Corona Borealis, 816.4 light-years from the Sun.
| Constellation | Corona Borealis |
|---|---|
| Distance | 816.4 light-years (250.3 pc) |
| Apparent magnitude | magnitude 6.39 |
| Absolute magnitude | magnitude −0.60 |
| Spectral type | K0 |
| Surface temperature | 4,190 K |
| Luminosity | 351 L☉ |
| Radius | 35.5 R☉ |
| Mass | 4.85 M☉ (estimated) |
| Right ascension (J2000) | 16h 12m 06.5s |
| Declination (J2000) | +39° 03′ 20″ |
| Space velocity (relative to the Sun) | 30.2 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.39). 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 1210. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 14 million years.
The Sun seen from there
From a planet around HIP 79385, the Sun would look like a star of magnitude 11.82, in the direction where our sky has the constellation Eridanus. It would be invisible to the naked eye.
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.