Star · B6V
HIP 29728
HIP 29728 is a main-sequence star of spectral type B6V in the constellation Orion, 701.7 light-years from the Sun.
| Constellation | Orion |
|---|---|
| Distance | 701.7 light-years (215.1 pc) |
| Apparent magnitude | magnitude 6.07 |
| Absolute magnitude | magnitude −0.59 |
| Spectral type | B6V |
| Surface temperature | 11,990 K |
| Luminosity | 282 L☉ |
| Radius | 3.89 R☉ |
| Mass | 4.55 M☉ (estimated) |
| Right ascension (J2000) | 6h 15m 40.2s |
| Declination (J2000) | +6° 03′ 58″ |
| Space velocity (relative to the Sun) | 31.2 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.07). Visible from the whole Northern Hemisphere and south to latitude 84° S. 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 1324. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 12 million years.
The Sun seen from there
From a planet around HIP 29728, the Sun would look like a star of magnitude 11.49, in the direction where our sky has the constellation Serpens. 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.