Star · A3V
HIP 24902
HIP 24902 is a main-sequence star of spectral type A3V in the constellation Auriga, 244.3 light-years from the Sun.
| Constellation | Auriga |
|---|---|
| Distance | 244.3 light-years (74.9 pc) |
| Apparent magnitude | magnitude 5.46 |
| Absolute magnitude | magnitude 1.09 |
| Spectral type | A3V |
| Surface temperature | 8,820 K |
| Luminosity | 36.5 L☉ |
| Radius | 2.59 R☉ |
| Mass | 2.54 M☉ (estimated) |
| Right ascension (J2000) | 5h 20m 14.7s |
| Declination (J2000) | +41° 05′ 10″ |
| Space velocity (relative to the Sun) | 31.0 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.46). Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N it never sets. It stands highest at midnight in December, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1782. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.3 million years.
The Sun seen from there
From a planet around HIP 24902, the Sun would look like a star of magnitude 9.20, in the direction where our sky has the constellation Scorpius. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 26080 15.2 light-years
- Haedus 15.9 light-years
- HIP 26310 18.8 light-years
- HIP 26957 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.