Star · B0IV
HIP 34301
HIP 34301 is a subgiant star of spectral type B0IV in the constellation Canis Major, 3,048 light-years from the Sun.
| Constellation | Canis Major |
|---|---|
| Distance | 3,048 light-years (934.6 pc) |
| Apparent magnitude | magnitude 5.41 |
| Absolute magnitude | magnitude −4.44 |
| Spectral type | B0IV |
| Surface temperature | 9,730 K |
| Luminosity | 6,770 L☉ |
| Radius | 28.9 R☉ |
| Mass | 11.3 M☉ (estimated) |
| Right ascension (J2000) | 7h 06m 40.8s |
| Declination (J2000) | −11° 17′ 38″ |
| Space velocity (relative to the Sun) | 33.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.41). Visible from the whole Southern Hemisphere and north to latitude 79° N. South of latitude 79° S it never sets. 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 1023 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 54 million years.
The Sun seen from there
From a planet around HIP 34301, the Sun would look like a star of magnitude 14.68, 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.