Star · A0V
HIP 49259
HIP 49259 is a main-sequence star of spectral type A0V in the constellation Vela, 291.4 light-years from the Sun.
| Constellation | Vela |
|---|---|
| Distance | 291.4 light-years (89.3 pc) |
| Apparent magnitude | magnitude 6.11 |
| Absolute magnitude | magnitude 1.35 |
| Spectral type | A0V |
| Surface temperature | 9,640 K |
| Luminosity | 32 L☉ |
| Radius | 2.03 R☉ |
| Mass | 2.45 M☉ (estimated) |
| Right ascension (J2000) | 10h 03m 20.6s |
| Declination (J2000) | −46° 38′ 10″ |
| Space velocity (relative to the Sun) | 12.7 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.11). 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 1735. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.2 million years.
The Sun seen from there
From a planet around HIP 49259, the Sun would look like a star of magnitude 9.59, 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 49878 15.4 light-years
- HIP 49736 17.7 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.