Star · M0III
HIP 20376
HIP 20376 is a giant star of spectral type M0III in the constellation Camelopardalis, 607.2 light-years from the Sun.
| Constellation | Camelopardalis |
|---|---|
| Distance | 607.2 light-years (186.2 pc) |
| Apparent magnitude | magnitude 5.40 |
| Absolute magnitude | magnitude −0.95 |
| Spectral type | M0III |
| Surface temperature | 3,800 K |
| Luminosity | 750 L☉ |
| Radius | 63.3 R☉ |
| Mass | 6.02 M☉ (estimated) |
| Right ascension (J2000) | 4h 21m 47.7s |
| Declination (J2000) | +60° 44′ 08″ |
| Space velocity (relative to the Sun) | 114.8 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.40). Visible from the whole Northern Hemisphere and south to latitude 29° S. North of latitude 29° N it never sets. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1419. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 11 million years.
The Sun seen from there
From a planet around HIP 20376, the Sun would look like a star of magnitude 11.18, in the direction where our sky has the constellation Triangulum Australe. 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.