Star · K5III
HIP 66251
HIP 66251 is a giant star of spectral type K5III in the constellation Camelopardalis, 903.7 light-years from the Sun.
| Constellation | Camelopardalis |
|---|---|
| Distance | 903.7 light-years (277.1 pc) |
| Apparent magnitude | magnitude 6.46 |
| Absolute magnitude | magnitude −0.75 |
| Spectral type | K5III |
| Surface temperature | 3,690 K |
| Luminosity | 731 L☉ |
| Radius | 66.2 R☉ |
| Mass | 5.98 M☉ (estimated) |
| Right ascension (J2000) | 13h 34m 42.8s |
| Declination (J2000) | +76° 32′ 48″ |
| Space velocity (relative to the Sun) | 35.4 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.46). Visible from the whole Northern Hemisphere and south to latitude 13° S. North of latitude 13° N it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1122. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 16 million years.
The Sun seen from there
From a planet around HIP 66251, the Sun would look like a star of magnitude 12.04, in the direction where our sky has the constellation Hydrus. 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.