Star · ?
HIP 36055
HIP 36055 is a supergiant star of spectral type ? in the constellation Monoceros, 1,887 light-years from the Sun.
| Constellation | Monoceros |
|---|---|
| Distance | 1,887 light-years (578.4 pc) |
| Apparent magnitude | magnitude 5.98 |
| Absolute magnitude | magnitude −2.83 |
| Spectral type | ? |
| Surface temperature | 4,990 K |
| Luminosity | 1,600 L☉ |
| Radius | 53.4 R☉ |
| Mass | 7.48 M☉ (estimated) |
| Right ascension (J2000) | 7h 25m 51.2s |
| Declination (J2000) | −5° 46′ 30″ |
| Space velocity (relative to the Sun) | 21.8 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.98). Visible from the whole Southern Hemisphere and north to latitude 84° N. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 139. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 33 million years.
The Sun seen from there
From a planet around HIP 36055, the Sun would look like a star of magnitude 13.64, in the direction where our sky has the constellation Aquila. 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.