Star · K1III
HIP 28829
HIP 28829 is a giant star of spectral type K1III in the constellation Camelopardalis, 451.4 light-years from the Sun.
| Constellation | Camelopardalis |
|---|---|
| Distance | 451.4 light-years (138.4 pc) |
| Apparent magnitude | magnitude 6.32 |
| Absolute magnitude | magnitude 0.61 |
| Spectral type | K1III |
| Surface temperature | 4,480 K |
| Luminosity | 90.1 L☉ |
| Radius | 15.8 R☉ |
| Mass | 3.29 M☉ (estimated) |
| Right ascension (J2000) | 6h 05m 08.2s |
| Declination (J2000) | +59° 23′ 36″ |
| Space velocity (relative to the Sun) | 44.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.32). Visible from the whole Northern Hemisphere and south to latitude 31° S. North of latitude 31° N it never sets. It stands highest at midnight in December, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1575. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 8.0 million years.
The Sun seen from there
From a planet around HIP 28829, the Sun would look like a star of magnitude 10.54, in the direction where our sky has the constellation Pavo. 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.