Star · B3IV
α Tel
α Tel is a subgiant star of spectral type B3IV in the constellation Telescopium, 279.5 light-years from the Sun.
| Other names | HIP 90422 |
|---|---|
| Constellation | Telescopium |
| Distance | 279.5 light-years (85.7 pc) |
| Apparent magnitude | magnitude 3.49 |
| Absolute magnitude | magnitude −1.17 |
| Spectral type | B3IV |
| Surface temperature | 13,100 K |
| Luminosity | 576 L☉ |
| Radius | 4.66 R☉ |
| Mass | 5.59 M☉ (estimated) |
| Right ascension (J2000) | 18h 26m 58.4s |
| Declination (J2000) | −45° 58′ 06″ |
| Space velocity (relative to the Sun) | 22.8 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 3.49). Visible from the whole Southern Hemisphere and north to latitude 44° N. South of latitude 44° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1747. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.0 million years.
The Sun seen from there
From a planet around α Tel, the Sun would look like a star of magnitude 9.49, in the direction where our sky has the constellation Auriga. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 90563 10.2 light-years
- HIP 90414 16.0 light-years
- HIP 91844 16.4 light-years
- HIP 90892 18.0 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.