Star · K0IV
HIP 49485
HIP 49485 is a subgiant star of spectral type K0IV in the constellation Vela, 267.6 light-years from the Sun.
| Constellation | Vela |
|---|---|
| Distance | 267.6 light-years (82.0 pc) |
| Apparent magnitude | magnitude 5.06 |
| Absolute magnitude | magnitude 0.49 |
| Spectral type | K0IV |
| Surface temperature | 5,050 K |
| Luminosity | 73.3 L☉ |
| Radius | 11.2 R☉ |
| Mass | 3.1 M☉ (estimated) |
| Right ascension (J2000) | 10h 06m 11.2s |
| Declination (J2000) | −47° 22′ 12″ |
| Space velocity (relative to the Sun) | 32.7 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.06). Visible from the whole Southern Hemisphere and north to latitude 43° N. South of latitude 43° S it never sets. It stands highest at midnight in February, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1758. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.7 million years.
The Sun seen from there
From a planet around HIP 49485, the Sun would look like a star of magnitude 9.40, in the direction where our sky has the constellation Lacerta. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 49736 7.98 light-years
- HIP 48583 13.2 light-years
- HIP 49714 16.1 light-years
- HIP 48241 19.9 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.