Star · A0III
HIP 36019
HIP 36019 is a giant star of spectral type A0III in the constellation Camelopardalis, 761.0 light-years from the Sun.
| Constellation | Camelopardalis |
|---|---|
| Distance | 761.0 light-years (233.3 pc) |
| Apparent magnitude | magnitude 6.30 |
| Absolute magnitude | magnitude −0.54 |
| Spectral type | A0III |
| Surface temperature | 10,530 K |
| Luminosity | 211 L☉ |
| Radius | 4.36 R☉ |
| Mass | 4.19 M☉ (estimated) |
| Right ascension (J2000) | 7h 25m 21.9s |
| Declination (J2000) | +81° 15′ 27″ |
| Space velocity (relative to the Sun) | 32.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.30). Visible from the whole Northern Hemisphere and south to latitude 9° S. North of latitude 9° N it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1265. 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 36019, the Sun would look like a star of magnitude 11.67, in the direction where our sky has the constellation Octans. 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.